G010-011: This is LFT 792, a known white dwarf. Spectrum DC according to Luyten (1952ApJ...116..283L).
G011-033: White dwarf suspect. The color estimate is somewhat uncertain due to the faintness of the star. [added comment: identified as a plate flaw by Bakos et al (2002ApJS..141..187B); the photometry by Eggen almost certainly applies to the K dwarf star near the nominal position (2MASS J12002514-0406010).]
G013-044: This star is a 7" double; the magnitudes are about 14 and 15, and both components appear to be red dwarfs.
G013-050: This is BD-04 3319. A companion of the 11th magnitude accompanies the star at 9" distance; this is obscured by the image of the large star on the Lowell plates and is therefore not listed separately. The companion is LTT 4814.
G014-046, G014-047: These form a common proper motion pair, separation 200".
G014-055: This star is a 10" double; the companion is about 15th magnitude and is a red dwarf.
G014-057, G014-058: These two stars are separated by about 8'.4, and although the measured motions are not precisely identical, a physical connection seems very probable. The brighter star is the known white dwarf Wolf 485 of spectral type DA. The faint star is a red dwarf.
G014-059: The 10th magnitude star BD-07 3635 = LTT 5222 is about 30" south-preceding. According to Luyten these two stars form a moving pair. On the Lowell plates, however, the larger star appears to have a noticeably smaller motion, and the measured position angles differ by about 30°. The fainter component only is therefore listed in our catalog. The possibility of a binary system should not be overlooked. [added comment: the stars indeed have common proper motion.]
G017-015, G017-016: These appear to share a common motion; the separation is 20".
G017-025, G017-027: The bright star is BD-03 3968. The faint star is 19'.5 distant, but appears to share the same motion.
G019-013, G019-014: These form a wide pair of 185" sharing common motion. The primary star is GC 23043, spectrum K6 according to Luyten.
G019-015: LFT 1324; this star is a very close double of 0".5 according to Luyten.
G020-016: This star is given as a double by Luyten (LTT 7093 and LTT 7094), magnitudes 15 and 15.5, separation 5".
G021-006: Announced as a probable white dwarf by Luyten on HAC 648 (1943HarAC.648....2L) with color index of +0.1. Greenstein finds this star to be a dwarf K (private communication, cf 1965ApJ...142..925E).
G021-008: This star is given as a double by Luyten (LTT 7271 and LTT 7272), separation 4".
G021-016: Announced as a probable white dwarf by Luyten on HAC 1280 (1954HarAC1280....2L) with color index of +0.3. Verified as a white dwarf by Greenstein in 1960. He writes: star G021-16 is a white dwarf with rather sharp lines, meaning actually that it is probably somewhat yellowish, perhaps early F in color. It shows, however, only the hydrogen lines, which is quite conventional for cooler white dwarfs (private communication, cf 1965ApJ...141...83E).
G022-008, G022-009: The brighter star is BD-04 4636. The faint companion is 33" distant and was announced by Luyten as a probable white dwarf on HAC 648 (1943HarAC.648....2L), color index +0.2. Greenstein (1960, private communication) gives the types as dwarf G and dwarf K.
G022-011: Announced as a probable white dwarf by Luyten on HAC 648 (1943HarAC.648....2L) with color index +0.4.
G026-005: This star is given as a close double by Luyten, separation 1".5.
G026-031: This is the known white dwarf L 930-80, spectrum DB0 according to Luyten (1952ApJ...116..283L).
G027-014: This star is a close double according to Luyten: magnitudes 13.9 and 15.5, separation 1".9. The brighter star is red, color of the companion is as yet undetermined.
G027-025, G027-026: These two stars appear to form a common proper motion pair with a separation of about 83". Luyten lists one star as LTT 9010, which is apparently identical with G027-026. No companion mentioned.
G028-013: Suspected white dwarf. Verified as a white dwarf by Greenstein (1961, cf 1975ApJ...196L.117G). The spectrum is DA.
G031-034: This is LDS 4, a double of 7".5 separation.
G053-038: White dwarf suspect.
G062-031, G062-032: Refer to G014-046 and G014-047.
G064-024: This star is a very close double; the magnitudes are about 11.5 and 12, the separation is 0".1.
G064-038: The measured motion is highly uncertain, as the images are near the limit of visibility. A check of two other pairs of plates seems to verify the motion, though the images are equally faint and diffuse on all plates. A possible companion lies about 21" distant in pa 305°. The motion of this object is somewhat less than that of the larger star, and in the opposite direction. The images are so uncertain that no real measurements are possible. [added comment: the motion is essentially correct; the companion, however, has near-zero motion.]
G064-043: Suspected white dwarf.
G070-004: This is the primary of the double star ADS 608 = Σ53. Aitken gives the magnitudes as 9.0 and 9.7 with a separation of 31".6 in pa 346°(1922). The two stars appear to form an optical pair only, as the companion shows no detectable motion on the Lowell plates. The separation and position angle are increasing slowly due to the motion of the primary.
G070-008: This is the faint companion to the 7th magnitude star LTT 417 = BD-00 109. The separation is 55", same motion and direction. The primary is above the magnitude limit of our survey, and is therefore not listed.
G070-050: These form the double star ADS 1057; the separation is 27" in pa 209°. Aitken gives the magnitudes as 8.3 and 10.0, and states that the measures of the pair have shown no change in 30 years.
G075-039: White dwarf suspect.
G077-024: The motion of this star is somewhat uncertain, as the images are very faint, and one of the first epoch images is partly obscured by a plate defect.
G082-022, G082-023: These two stars, separated by 2'.8, appear to show approximately the same motion, but the position angles differ by about 30°. [added comment: modern astrometry shows the stars to have significantly different proper motions.]
G082-038: The motion of this star is somewhat uncertain due to the faintness of the images, and due to the fact that the star appears peculiarly diffuse and nebulous on the first epoch plates taken January 1932. The reality of a motion of about 0".5 per year seems to be verified by a check of several sets of plates, however, and the star appears to be quite red.
G084-006: The star was noted as slightly bluish by both observers. Luyten's estimated color class is 'f', and the star is thus a possible white dwarf suspect.
G084-026: White dwarf suspect.
G084-045: This is the close double star ADS 3900. The companion (not listed separately) is magnitude 13, about 4" distant from the primary. The two stars show the same motion and probably form a long-period binary.
G092-011, G092-014: These two stars may form a wide moving pair, although the measured motions are not precisely identical. The separation is approximately 20'. [added comment: modern astrometry shows the motions are significantly different.]
G092-040: This is LFT 1503, a known white dwarf. The spectrum is DA according to Luyten (1940HarAC.527....1L).
G093-028: The southern LTT catalog reports a spectral type of G0.
G093-053: This star was announced as a possible white dwarf by Luyten HAC 1280 (1954HarAC1280....2L). The color index as determined by Luyten is equivalent to that of an A0 star. Verified by Greenstein (1960, cf 1965ApJ...141...83E). The spectrum is DA.
G099-037: White dwarf suspect.
G099-044: This faint star has the largest new motion detected in the first 100 regions of the Lowell survey. The color does not appear to be noticeably blue, but neither is it definitely red. We are therefore assuming it is a white dwarf suspect of later than usual spectral type. See also 1960BOTT....2s..16H, star Name HL 4.
G106-012: Refer to G099-044. Luyten (1963POMin..13....1L) finds a parallax of 0".148; Herbig's spectrum = DK.
G106-049: This is Ross 614, for many years a well known astrometric binary. The faint companion was first detected with the 200-inch telescope in 1955 and is now recognized as one of the faintest and least massive of all known stars (cf 1955S&T....14..364L and 1955AJ.....60..379L).
G106-053, G106-054: These two stars may form a wide moving pair, although the measured position angles differ by about 12°. The separation is approximately 7'.5. [added comment: modern astrometry shows the pair to have common proper motion with separation of 434" in pa 169°.]
G108-007, G108-008: Refer to G106-053 and G106-054.
G108-013: The faint images of this star appear unusually diffuse on the Lowell plates, but the motion appears to be verified by a check of a second pair of plates. The star is quite red.
G108-020: A possible companion star of the 16th magnitude lies at a distance of about 88" in pa 200°. The motion of this object is only about 0".2 per year, but in approximately the same direction as G108-20. [added comment: modern astrometry shows motion of only 0".12 per year for the companion.]
G108-047: The images of this star are near the plate limit, but the motion appears to be verified by a check of a second pair of plates.
G112-037, G112-038: These two bright stars for a common proper motion pair with a separation of about 58".
G113-007: This is the double star ADS 6487. Aitken gives the individual magnitudes as 8.3 and 13.8, with a separation of 2".2 (1919). The two stars form a physical system, but a third star, C, is independent.
G113-026, G113-027: These two faint stars form a common proper motion pair with a separation of about 22".
G113-042, G113-043: This is the common proper motion pair LDS 221. The separation is about 87".
G124-024: This is GC 19326. The star has a companion of the 16th magnitude (LFT 1093) located 15" distant. The companion is obscured by the image of the bright star on the Lowell plates, and is therefore not listed in our catalog.
G124-026: White dwarf suspect.
G124-043, G124-044: A common proper motion pair with a separation of 15". Both stars are very red.
G124-049: This star seems to be identical with LTT 5739, but Luyten's position angle is 289°, possibly a misprint for 189°. Our value of 201°was remeasured.
G124-053: This is LDS 493. According to Luyten, the components are magnitudes 15.3 and 15.7 with a separation of 7". [added comment: not double — LDS 493 lies 1m RA east.]
G151-003: The motion of this faint star is uncertain and cannot be verified at Lowell because only one first epoch plate is available. [modern astrometry shows motion 0".31 per year in pa 246°.]
G151-019, G151-021: These two stars form a common proper motion pair with a separation of 48".
G151-030, G151-032: According to Luyten these two stars form a common motion pair (LDS 518) with a separation of 677".
G151-061: Refer to note on G151-062 and G151-063.
G151-062, G151-063: A common proper motion pair with a separation of about 55". These are BD-08 3981 and BD-08 3983. The faint star G151-061 shows approximately the same motion and may be a distant member of the system. The separation from the bright pair is 20'.2.
G152-013: A star of magnitude 12.5 at about 225" following has a motion of about 0".2 per year in pa 240°. This star appears to be BPM 77814.
G152-025: A possible white dwarf suspect.
G152-026: This faint star may be a distant companion to the bright pair G152-027 and G152-028. Refer to note on G151-062 and G151-063.
G152-027, G152-028: Refer to G151-062 and G151-063.
G152-031, G152-032: A common proper motion pair with a separation of about 13".
G152-060: This seems to be the same star as LTT 6335, but there is a discrepancy of 1m in the Right Ascension, which Luyten gives as 15h50m.5 (equinox 1950).
G153-025: This appears to be the same star as LTT 6431, identified by Luyten as BD-05 4242. A check of our plates shows that the motion star is about 7' south of the BD star, and the motion star itself has no BD number.
G153-027: An independent discovery of this star is reported by L. Plaut (1962PASP...74..162P).
G153-028: While making the finding chart for this star, a 15th magnitude companion was detected which appears to share the motion of the primary. The faint star is located 16" distant in pa 5°. Both stars are indicated by the identifying lines on the chart.
G153-040: Luyten's estimated color class for star is 'a'.
G153-041: This is a known white dwarf L 770-3. The spectrum is DA according to Greenstein (1957ApJ...126...19G).
G153-051, G153-052: A common proper motion pair with a separation of about 10".
G153-060: This is LTT 6586, but we find the BD number to be BD-03 3954.
G153-061, G153-062: These form the common proper motion pair LDS 563. The separation is about 128".
G153-067: A faint companion to this star was detected on an earlier region (G17), but falls just off the edge of the plate on G153. The separation is about 19'.5. Refer to G017-025 and G017-027.
G154-012: The motion of this star is somewhat uncertain since the object assumed to be the first epoch image is 1.5 magnitudes faint than the second epoch images. There are thus two possible interpretations: the object may be a single motion star and a variable; or there may be two faint variables with a 10" separation. [added comment: this is V504 Sgr, a Mira variable (not a short-period Cepheid) with near-zero proper motion.]
G154-019: White dwarf suspect.
G154-023: White dwarf suspect.
G154-024: This is the close double star LDS 613. Refer to G020-016.
G154-032: This is the double star ADS 10858 or Σ3128. Aitken gives the magnitudes as 7.0 and 10.5, with a separation of 1".2 (1886). The components evidently form a physical pair. A measurement by van den Bos (1963) shows a position angle increase of 43°since 1886, and the separation is now about 0".5.
G154-036: This is the double star ADS 10938 or Hu 190. Aitken gives the magnitudes as 9.2 and 10.5 with a separation of 0".5 (1922). A measurement by van den Bos (1963) shows the position angle has decreased by 69° since 1900, while the separation has not changed significantly.
G154-038, G154-039: These form the common proper motion pair LDS 621. The separation is about 8".
G154-045: No color measurement could be obtained for this star because the image is lost in the bright image of a nearby star on the red plate.
G155-015: White dwarf suspect.
G155-017: This star shows approximately the same motion as G155-026, but the separation is 2.6°.
G155-019: White dwarf suspect.
G155-025: This faint star seems to show approximately the same motion as the 4th magnitude star α Sct, which is located about 16'.6 to the east.
G155-026: Refer to note on G155-017.
G155-034: White dwarf suspect. Luyten's estimated color for the star, however, is 'g'; and there is also a discrepancy in the motion, which Luyten finds to be 0".23. A check of the plates shows no other motion star in the immediate area.
G155-039: This is BD-14 5187. It is the double star Rossiter 4596; the companion is a 12th magnitude star at 6".
G155-043: This star was noted as slightly bluish by both observers. Luyten's estimated color is 'f'. A possible white dwarf suspect.
G156-002, G156-003: Refer to G027-025 and G027-026.
G156-012, G156-013: A common proper motion pair with a separation of about 33".
G156-022, G156-023: A common proper motion pair with a separation of about 38".
G156-029: The images of this star have a peculiar elongated appearance on the Lowell plates, suggesting that the image of the motion star is partly fused with the image of a nearby field star. The motion and color measurements are therefore somewhat uncertain. Luyten reports a dM spectrum in his Bruce catalog. [added comment: there is also a mag 18 common-motion companion 19" in pa 294°.]
G156-034, G156-035: A common proper motion pair with a separation of about 139". The primary is the visual double star ADS 16145 or Σ2928. Aitken gives the individual magnitudes as 8.0 and 8.0 with a separation of 4" (1924). The position angle between the components has decreased by about 20°in the last century.
G156-036, G156-037: A common proper motion pair with a separation of about 10".
G156-048: This is the close double star ADS 16720 or Σ2944. Aitken gives the magnitudes as 7.0 and 7.5 with a separation of 3".1 (1925). The position angle between the components is increasing slowly.
G156-052, G156-053, G156-054: These stars appear to form a moving triple group. G156-53 and G156-54 form a close pair with a separation of about 7". The third star, G156-52, is at a distance of about 78". All three stars seem to be quite red.
G156-056: The southern LTT catalog reports a spectral type of G0.
G156-064, G156-065: The bright star is BD-08 5980. The newly discovered companion is at a distance of 43", and appears to share the motion. The color of the faint star seems definitely bluish.
G157-032, G157-033: These form a common proper motion pair ADS 16611 (or Σ2993) with a separation of about 26".
G157-034: This is L 935-50. Our color estimate of '0' agrees with Luyten's color class of 'a'. Suspected white dwarf.
G157-035: The color of this star is somewhat uncertain due to the faintness of the images on the Lowell plates, but does not appear to be at all reddish. A white dwarf suspect.
G157-036: This star is a close double with a separation of about 0".6 (1916); and a physical companion to the bright star 91 Aqr, which is located 49" distant. All three stars share the large proper motion, but the 4th magnitude is above the magnitude limit of our survey and is therefore not listed in our catalog. The Yale motion for the primary is 0".38 in pa 92°.
G157-041: This is the double star ADS 16649 or β79. Aitken gives the individual magnitudes as 8.0 and 9.6 with a separation of about 1".9 (1925). The position angle between the components has been decreasing slowly from 115°in 1876 to 59°in 1925, but the exact period is still uncertain.
G157-066: The measured motion and color of this star are somewhat uncertain since the second epoch image is fused with the image of a 15th magnitude field star.
G157-072: This faint star was noted as slightly bluish by both observers. A possible white dwarf suspect.
G157-082: White dwarf suspect.
G158-010: This is the double star ADS 17107 or Σ3046. Aitken gives the magnitudes as 8.0 and 8.5 with a separation of about 3".0 (1926). The position angle between the components is increasing slowly.
G158-012, G158-113: A common proper motion pair with a separation of about 31".
G158-027: This faint star has the largest new motion detected up to this point in the survey. The color is strongly red. A parallax has been obtained at the U.S. Naval Observatory, giving π= 0".212; the absolute visual magnitude is then 15.36 (1975PUSNO..24a...1H).
G158-039: Suspected white dwarf.
G158-045: Suspected white dwarf. This is PHL 6421.
G158-053: A parallax has been obtained at the U.S. Naval Observatory, giving π= 0".026; the absolute visual magnitude is then 11.02 (1978PUSNO..24d...1H).
G158-054, G158-057: These two faint stars may form a wide proper motion pair. The separation is about 5'.1.
G158-068: Luyten lists this star as a triple system; AB = mag 15.4 and 15.6, separation 25" in pa 255°; AC = 25" in pa 289°. No evidence for the AB duplicity can be found on Lowell plates, although a pair of these magnitudes and separation should be clearly obvious. The reality of the C component, listed as magnitude 21+, cannot be confirmed on Lowell plates. Star B is LP 645-12; star C is called LP 645-10. [added comment: the AB pair are 4".5 apart not 25", and thus not resolved on the Lowell plates for that reason.]
G158-073, G158-074: A common proper motion pair with a separation of about 14".
G158-076: This is LP 645-82. Luyten reports a companion that he designates LP 645-83. Magnitude 16.8, separation 11" in pa 28°.
G158-077, G158-078: A common proper motion pair with a separation of about 90". The fainter component is a confirmed white dwarf, spectrum DA (1965ApJ...142..925E).
G158-086, G158-087: A common proper motion pair with a separation of about 50".
G158-093: Luyten reports a companion, designated LP 645-39. Magnitude 17.6, separation 20".5 in pa 108°.
G158-095: A paralax has been obtained at the U.S. Naval Observatory, giving π= 0".060; the absolute visual magnitude is then 11.64 (1972PUSNO..20f...1R).
G158-097, G158-098: These may share a common proper motion, though the measured values are not precisely identical. The bright star is the triple system ADS 450, consisting of a 0".2 pair with a 10.5-year period, and a third component of magnitude 12.5 at a distance of 2".2. G158-97 may thus be the fourth known member of this interesting multiple system. It is approximately 7'.1 distant from the bright primary. [added comment: modern astrometry shows G158-97 indeed shares a common motion with the ADS 450 system; the separation is 431" in pa 351°.]
G158-100: This is LTT 300. We obtain a color measurement of '0' for this star and are therefore listing it as a white dwarf suspect. Luyten's color class for this star, however, is 'm'.
G158-107: Luyten lists a faint star that may be a companion to G158-107, lying 9s east and 2'.4 south. Called LP 764-29, it is stated to be magnitude 19.6 photographic.
G158-114: We have identified this star with LP 704-91. Luyten lists another pair, LP 704-11 and LP 704-12, at nearly the same position, stated to be a 2" pair in pa 295°. Both entries may refer to the same object, as Luyten gives the same number L 865-48 as a reference for both.
G158-120: This is also BD-13 6504.
G158-122: Luyten reports this to be a pair of 2" separation in pa 72°. The companion, designated LP 704-32, is stated to be of magnitude 15.6.
G158-128: Suspected white dwarf.
G158-132: Suspected white dwarf.
G158-134: Suspected white dwarf.
G158-138: This may be a distant companion to G158-35, which lies 4'.3 distant, nearly due south (pa 188°). Both objects are indicated on the G158-138 identification chart; G158-35 is the encircled image. [added comment: the pair is confirmed to have common proper motion.]
G158-144: A noticeably bluish star (color estimate = 0) lies in the field 42" distant in pa 225°, magnitude 16.2. It is the first star to the lower-right of the motion star on the identification chart. The bluish star shows no certain motion on the Lowell plates.
G158-146: We have identified this as LP 764-107, though there is a discrepancy in the position, which Luyten gives as 0h15m08s -14°54'.4 (1950).
G158-166: This is LP 705-47. Luyten states "has a very faint preceding companion, may be optical." [added comment: the companion is indeed an optical one.]
G158-167: White dwarf suspect.
G158-171: Luyten lists a faint star with a similar motion some 12' distant toward the north; the may possibly form a wide pair. Designated LP 705-67, it is stated to be magnitude 16.0 with a motion of 0".205 in pa 102°. A possible faint image exists at this position on the Lowell plates, but too uncertain for measurement.
G159-031: White dwarf suspect.
G159-035: This star shares the proper motion of GC 2548 = Ci 20 147 = HD 13043, which lies 77" to the southeast. The primary is magnitude 6.9, spectrum G1.
G160-051: Suspected white dwarf.
G160-053: The motion of this faint star is somewhat uncertain since the images are at the plate limit.
G160-060: This is the white dwarf companion to 40 Eri, a system so well known as to require no further description here.
G161-009: This faint star was noted as slightly bluish by both observers. A possible white dwarf suspect.
G161-019, G161-020: A common proper motion pair with a separation of about 15".
G161-024: The LFT catalog reports a spectral type of K2.
G161-033, G161-034: A common proper motion pair with a separation of about 38".
G161-036, G161-037: A common proper motion pair with a separation of about 19". The primary is a white dwarf suspect.
G161-049, G161-050: A common proper motion pair with a separation of about 92".
G161-056: The color estimate of only +1 on a 16th magnitude motion star makes this an interesting object. It may be a white dwarf of rather late spectral type.
G161-068: Suspected white dwarf.
G161-075, G161-076: These two stars form the moving double LDS 281. The separation is about 10".
G162-035, G162-036: These two stars form the common proper motion pair LDS 300. The separation is about 18".
G162-066: This is LTT 3870. Luyten's color class for this star is 'a'.
G163-027: This is the known white dwarf LFT 753. The spectrum is DA according to Luyten (1952ApJ...116..283L).
G163-028: White dwarf suspect.
G163-039, G163-040: These two stars form the common proper motion pair LDS 330. The separation is about 17".
G163-050, G163-051: These two stars form a wide motion pair with a separation of about 4'.7. The primary is the known white dwarf L 970-30 with a DA spectrum.
G266-003: This star may possibly be a late-type white dwarf or subdwarf.
G266-012: A faint companion to this star was detected on the earlier region G158, where the two were designated G158-012 and G158-013. The companion is magnitude 16.5, separation 27" in pa 131°. This pair also has the designation LDS 831.
G266-029: This is the double star ADS 17173 or B 630. van den Bos (1963) obtained a separation of 0".15 in pa 348.4°, individual magnitudes 9.6 and 10.0. The Lick Observatory "Index Catalogue" entries indicate a considerable change in position angle since 1925, when a measurement of 26°was obtained. However, the measurements were difficult and uncertain owing to the closeness of this pair.
G266-031: Luyten finds this star to be a close pair, magnitudes 14.3 and 16.2, separation 6" in pa 126°.
G266-032: White dwarf suspect. This is PHL 639.
G266-034: Luyten reports a companion to this star, magnitude 18.3, designated LP 824-92.
G266-039, G266-040: These form a common proper motion pair (LDS 833) with a separation of 7" in pa 326°.
G266-052: This appears to be BPM 46040, but Luyten's motion for the star is only 0".10.
G266-054: A possible white dwarf suspect.
G266-060, G266-061: These form the common proper motion pair LDS 1, separation about 9" in pa 172°.
G266-067, G266-068: These form the common proper motion pair LDS 5, separation about 43" in pa 3°.
G266-072: A possible white dwarf suspect.
G266-084, G266-085: These form the common proper motion pair LDS 10, separation about 17" in pa 249°.
G266-088, G266-089: These form the common proper motion pair LDS 12, separation about 8" in pa 328°.
G266-114: The correct CD reference for this star is CD-26 134, not CD-26 137 as given in the LTT catalog.
G266-115: This is ADS 366 or h1968. The ADS components are purely optical, however, and do not share the motion of the bright star.
G266-121, G266-122: These two stars form a common proper motion pair with a separation of about 33" in pa 150°.
G266-125, G266-126: These form a common proper motion pair with a separation of about 145" in pa 313°.
G266-135: White dwarf suspect.
G266-141: Possible white dwarf suspect. Luyten's color class for the star is 'g'.
G266-157: Possible white dwarf suspect. Luyten's color class for the star is 'g'.
G266-161, G266-162: These form a common proper motion pair with a separation of about 18" in pa 325°.
G267-007: This is LTT 9819, but there is a discrepancy in the position angle, which Luyten gives as 1°.
G267-014: This star was noted as slightly bluish by both observers. A possible white dwarf suspect.
G267-018: White dwarf suspect. Luyten's estimated color class is 'a-f'.
G267-025: This is GC 49 or Argentine General Catalogue 32416, the fifth largest proper motion known.
G267-032: Suspected white dwarf. This is Ton S 141 and PHL 671.
G267-033: Luyten reports a companion of magnitude 20.8, designated LP 880-441. Separation 8" in pa 8°.
G267-037: Suspected white dwarf. Luyten's color class for this star is 'g'.
G267-039: This star was noted as slightly bluish by both observers. A possible white dwarf suspect.
G267-044: The position of this star matches BPM 46067, but there are discrepancies in both motion and angle; Luyten obtains 0".04 in pa 32°.
G267-054, G267-055: This is the common proper motion pair LDS 5, separation about 44" in pa 2°. cf G266-067, G266-068.
G267-064: A white dwarf suspect.
G267-067: A white dwarf suspect.
G267-071, G267-072: Refer to G266-088, G266-089.
G267-087, G267-089: These form the common proper motion pair LDS 14, separation about 55" in pa 270°.
G267-091: This appears to be BPM 46259, but there is a discrepancy in the position angle, which Luyten gives as 260°.
G267-100: This appears to be BPM 46297, but there is a discrepancy in the position angle, which Luyten gives as 264°.
G267-106, G267-107: These form a common proper motion pair with a separation of about 51" in pa 292°.
G267-112: Suspected white dwarf.
G267-116: Luyten finds a faint companion to this star, which he designates LP 881-131. Separation 54" in pa 355°, magnitude 19.5.
G267-128: This is the visual double star h 3375, individual magnitudes 6.8 and 8.6 according to the Lick Observatory "Index Catalogue"; separation 5".3 in pa 168°(1954). Same motion and direction.
G267-141: This is the close double star I 705. The Lick Observatory "Index Catalogue" gives the magnitudes as 7.7 and 7.9 with a separation of 0".1.
G267-153: This is Z Scl. The suspected variability of the star appears never to have been confirmed.
G267-158: This star seems to be BPM 46562; the position angle of 288°given by Luyten appears to be a 180° error.
G267-170, G267-171: These form a common proper motion pair with a separation of about 58" in pa 196°.
G267-172: The blue star PS 2-31 lies 8' to the south.
G268-040: Suspected white dwarf.
G268-046: This is LTT 442, but there is a discrepancy between our measurements and those of Luyten, who obtains 0".22 in pa 36°.
G268-048: This is the double star ADS 666. The Lick "Index Catalogue" gives the separation as 5".3 in pa 100° (1932), magnitudes 8.7 and 13.7. The large galaxy extending across the south edge of the finder chart is NGC 253.
G268-051, G268-052: These two stars form the common proper motion pair LDS 27; separation about 7" in pa 209°.
G268-060: This is LTT 490. Luyten reports a companion of magnitude 17.0, which designates LP 826-170. Separation 17" in pa 69°.
G268-062: This is the double star ADS 716. The Lick Observatory "Index Catalogue" gives the magnitudes as 7.7 and 8.4, separation 1".8 in pa 256°(1959). Both separation and position angle have been decreasing slowly during the past century. A third component at about 33" (1908) is not a physical member of the system.
G268-067: The correct BD number for this star is BD-15 162, not BD-14 162 as reported in the LTT catalog.
G268-074: Suspected white dwarf.
G268-083: This appears to be BPM 70454, but the motion reported in the BPM catalog is only 0".087.
G268-085: This is LTT 554, but there is a discrepancy in the position angle, which is is given in the LTT catalog as 113°.
G268-097, G268-098: These two stars for a common proper motion pair with a separation of about 28" in pa 127°.
G268-101: This is the common proper motion double star ADS 860. The Lick "Index Catalogue" gives the separation as 5" in pa pa318°, magnitudes 8.2 and 10.2.
G268-110: This large new motion is nearly equal and parallel to G268-135 (LFT 118), which lies about 2°distant. The divergence of the measured position angles would indicate an approach of the moving pair, which in turn would require a negative radial velocity. However, Gliese lists a positive value for LFT 118 (Gl 54.1), so it appears that the near-equality of motion is fortuitous. The other alternative, that of large errors in the position angle measures, appears unlikely for so large a motion, and cannot remove the divergence.
G268-115: A faint and distant motion companion to this star was detected on the overlapping region G269. Refer to G269-092, G269-095.
G268-142, G268-143: These two stars form the moving pair LDS 41. Separation about 18" in pa 173°.
G268-150: This is the double star ADS 1066; the most recent measurements in the Lick "Index Catalogue" give the separation as 1".6 in pa 308°(1959), magnitudes 9.0 and 9.4.
G269-032, G269-033: Refer to G267-170, G267-171.
G269-059: From his photometric measurements on this star, Eggen derives a Mv of +5.3 with a resultant large velocity component (W = -450 km/sec). There is a large discrepancy with our magnitude and color estimates, however, suggesting the possibility of misidentification of the star. The Eggen measurements may refer to the 15th magnitude star 1' preceding, which shows slight motion (0".08) on our plates in approximately the same position angle. Our color estimate for this star is +1 or +2.
G269-065: The correct CD number for this star is CD-38 327, not CD-37 358 as given in the LTT catalog.
G269-070: Suspected white dwarf. Luyten's estimated color class for the star is 'g'.
G269-074: Suspected white dwarf. Luyten's estimated color class for the star is 'f'.
G269-092, G269-095: These stars appear to form a wide common motion pair LDS 35, separation about 184" in pa 228°.
G269-093: Suspected white dwarf. This is PHL 984. Luyten's estimated color class for the star is 'a'.
G269-096, G269-097: A common proper motion pair, separation about 33" in pa 189°.
G269-100, G269-101: A common proper motion pair, separation about 39" in pa 122°.
G269-111: This is LP 882-316. Luyten finds a faint companion star, LP 882-315, magnitude 17.5, separation 5" in pa 337°.
G269-127: A star of 16th magnitude, about 20" to the north (pa about 350°) shows a measurable motion on the Lowell plates. We obtain an annual motion of about 0".11 in pa 123°, color +2.
G269-128, G269-129: This is the double star LDS 837, separation 7" in pa 83°.
G269-155: The correct CD number for this star is CD-26 466, not CD-26 467 as given in the LTT catalog.
G269-157, G269-158: A common proper motion pair; separation about 23" in pa 84°.
G269-160: Suspected white dwarf. Luyten's estimated color class for the star is 'f'.
G269-172: This appears to be LTT 812, though there is a discrepancy of about 5' in Declination, which the LTT catalog gives as -34°00' (1950).
G270-008: Possible white dwarf suspect. The star seemed somewhat bluer on the earlier region G158, where the color estimate was '0'. Refer to G158-100.
G270-021, G270-022: These two stars possibly form a wide common motion pair; the separation is about 190" in pa 76°. [added comment: modern astrometry shows the motions are not similar.]
G270-027: This is G268-017, but the previous identification with BPM 70284 was in error. The BPM object is about 1m preceding.
G270-032, G270-033: A common proper motion pair; separation about 6" in in pa 120°; the companion is newly listed.
G270-048: This is the white dwarf star Feige 7; Feige reports a photographic magnitude of 15.0 and a color index of -0.35. The star is also PHL 814.
G270-065, G270-066: These form a common proper motion pair with a separation of about 65" in pa 44°; the companion is here newly listed.
G270-075: The bright star on the left edge of the finder chart is 19 Cet; motion 0".32 in pa 226°.
G270-081: Possibly a late-type white dwarf or subdwarf.
G270-093: White dwarf suspect. This is PHL 3101, estimated U-V = -0.3.
G270-096: White dwarf suspect. This is PHL 3120, estimated U-V = -0.2.
G270-098: This is the white dwarf LTT 524 = PHL 6902; spectrum DA.
G270-115, G270-116: A common proper motion pair, separation about 31" in pa156°. This pair is also known as LDS 33.
G270-120, G270-121: Refer to G268-097, G268-098.
G270-123: White dwarf suspect. This is PHL 3287, estimated U-V = -0.3.
G270-124: White dwarf suspect. This is PHL 962, estimated U-B = -0.6, B-V = -0.3.
G270-126: Suspected white dwarf.
G270-139: This is G268-113. The previously published BD reference is in error: the star is not a BD star.
G270-143, G270-145: These two faint stars possibly form a wide common motion pair; the separation is about 196" in pa 304°. [added note: modern astrometry confirms the common motion.]
G270-154, G270-155: A common proper motion pair with a separation of about 8" in pa 149°, newly listed.
G270-167: Suspected white dwarf.
G270-172: This is the close double star Rossiter 4167; magnitudes 7.8 and 13.2; separation 1".7 in pa 306°(1943).
G270-176: This is the fainter component of the system 37 Cet; separation 49".7 in pa 331°.
G271-002, G271-003: Refer to G270-154, G270-155.
G271-010: Both observers recorded this star as being slightly bluish. Luyten's color class estimate, however, is 'k-m'.
G271-011: Both observers recorded this star as being slightly bluish.
G271-019: Suspected white dwarf.
G271-022, G271-023: These two stars for a common proper motion pair with a separation of about 194" in pa 335°, newly listed.
G271-027: This faint star appears slightly bluish on the Lowell plates. Luyten's estimated color class is 'f'.
G271-031, G271-032: Refer to G 70-50, G 70-51.
G271-047: Suspected white dwarf. Luyten's estimated color class is 'a'. Luyten also finds a companion of magnitude 19.8, designated LP 587-43; separation 9" in pa 264°.
G271-066, G271-067: These form a common proper motion pair with a separation of about 183" in pa 88°; the faint companion appears to be listed here for the first time.
G271-076, G271-077: These form a common proper motion pair with a separation of 8" in pa 252°, newly listed.
G271-081: Suspected white dwarf.
G271-094, G271-099: These two stars possibly form a wide common motion pair; the separation is 7'.2 in pa 22°; newly listed.
G271-105: Luyten finds this star to be a close pair; separation 4" in pa 260°, magnitudes 15.5 and 16.2.
G271-106: This is the white dwarf star Ross 548; spectrum DA. The star is also PHL 1062.
G271-111: Suspected white dwarf.
G271-114: The motion of 0".33 for this star is somewhat uncertain; the images are faint and indistinct.
G271-115: This is also PHL 7450, a white dwarf of spectral class DA.
G271-117: This is the white dwarf suspect PHL 1086. Luyten's estimated color class for the star is 'a'.
G271-134: This appears to be LTT 924, though there is a discrepancy in the Declination, which Luyten gives as -12°19' (1950); the star is also BPM 70772, where the Declination is given correctly.
G271-137: Both observers thought this star to be slightly bluish.
G271-139: Both observers thought this star to be slightly bluish.
G271-144, G271-145: These form a common proper motion pair with a separation of about 38" in pa 306°. The companion here is newly listed.
G271-158: Both observers thought this star to be slightly bluish.
G271-173, G271-174: These form the common proper motion pair LDS 58. Separation about 28" in pa 201°.
G272-008, G272-009: These two stars form the common proper motion pair LDS 46. Separation about 39" in pa 313°.
G272-012, G272-013: A common proper motion pair; separation about 80" in pa 153°. The companion appears to be a new discovery. [added note: the bright star in fact has small motion, but the companion shares common motion with another fainter star at 33" in pa 163°.]
G272-018: The position angle of this star is somewhat uncertain; noticeably different results are obtained by using different first-epoch plates. The reported value of 69°was measured with the plates appear to the most clearly defined images. [added comment: UCAC2 proper motion is 0".37 per year in pa 64°.]
G272-019, G272-020: These form a common proper motion pair with a separation of about 14" in pa 273°; the companion appears to be a new discovery.
G272-028: This appears to be LTT 823, but Luyten reports a much larger motion of 0".32 annually. A check of our plates shows no other large motion in the area, and confirms our motion of about 0".20.
G272-039: This is L 654-5. Luyten finds a common motion companion of magnitude 20.4 at 117" in pa 18°; the two stars form his pair {LDS 1103
G272-044: Both observers thought this faint star to be slightly bluish.
G272-055: Suspected white dwarf. This is L 726-007 and PHL 3499; Luyten's color class estimate is 'a'.
G272-060: Suspected white dwarf. This is LP 768-230 and PHL 3537. Luyten's color class estimate is 'a-f'.
G272-061: This is the well-known high proper motion pair L 726-008, a red dwarf binary system of visual magnitudes 12.4 and 13.0, separation about 2".4. The components (not listed separately) have the smallest masses yet determined for any visible star. The fainter component is the flare star UV Cet.
G272-074, G272-075: These two stars form a common proper motion pair; separation about 26" in pa 154°.
G272-095: This is LTT 961, but the listed BD number of BD-13 311 is in error; the correct BD number is BD-13 321.
G272-096: This appears to be LP 708-447, but there is a discrepancy in the magnitude, which Luyten gives as 13.8 photographic.
G272-097: Luyten reports a companion of magnitude 18.8 in pa 86°, separation 29". These form his pair LDS 1117.
G272-106: Suspected white dwarf. This is PHL 3878. Luyten's estimated color class is 'a-f'.
G272-112, G272-113: Refer to G271-173, G271-174.
G272-119, G272-120: These form the common proper motion pair LDS 59, also designated in a later Luyten catalog under the designation LDS 1120. The separation is about 28" in pa 220°. Luyten's magnitude listing for the fainter component in the LTT and BPM catalogs is evidently in error, and seems to refer to the bright field star about 30" from the primary, but in the opposite direction, toward pa 20°. The proper motion companion is a 16th magnitude object. Refer to the finder chart for this pair.
G272-121: Luyten reports a companion of magnitude 17.3, designated LP 828-77. Separation 14" in pa 317°.
G272-126, G272-127: These form the common proper motion pair LDS 60; separation about 29" in pa 137°.
G272-131: Luyten's estimated color class for this star is 'g'.
G272-132, G272-133: These form a common proper motion pair, newly discovered, with a separation of about 7" in pa 184°. Both stars seem to be extremely red.
G272-149: This appears to be BPM 70905, though Luyten has a considerably lower position angle of 54°.
G272-152: Suspected white dwarf.
G273-001: This is the close visual binary ADS 16644 or β182; the ADS catalog gives the individual magnitudes as 8.7 and 8.9 with a separation of 0".6 (1959). The position angle of this pair is increasing very slowly. A third faint star shares the proper motion of the system; this is VBS 12. It is 15" from the bright primary in pa 47°, magnitude about 17.
G273-007, G273-008: These form the common proper motion pair LDS 810; separation about 21" in pa 143°.
G273-011: Luyten reports a companion which he designates LP 822-15. Magnitude 17.8, separation 6" in pa 61°. The two stars for the pair LDS 2980.
G273-013: Suspected white dwarf. The star is PHL 459. Luyten's estimated color class is 'a'.
G273-014: There is some evidence for a slight variability of this star on the Lowell plates.
G273-019: The very blue star GD 1115 lies in the field about 52" distant from G273-19 in pa 229°.
G273-022: Luyten reports a companion of magnitude 21, which he designates LP 822-59. Separation 6" in pa 360°.
G273-026: Luyten finds a companion of magnitude 17.6, which he designates LP 822-66. Separation 5" in pa 4°.
G273-040: Suspected white dwarf. This star is PHL 506. Luyten's estimated color class is 'a'.
G273-050: This is LP 878-32. Luyten finds a companion of magnitude 19.7, which he designates LP 878-33. Separation 5" in pa 67°. Luyten's estimated color class for the primary is 'm'.
G273-067, G273-068: These two stars for the wide pair LDS 816; separation about 339" in pa 353°. The BD number listed under LDS 816 appears to be incorrect. The fainter star, G273-67, is the very close pair Voute 28, with a separation of about 0".2 (1962); Gliese (1969VeARI..22....1G).
G273-070, G273-071: These form the common motion pair LDS 2989; separation about 31" in pa 232°.
G273-077: The closest star on the finder chart (mag 12 at 14" in pa237°) shows some proper motion in very nearly the same position angle. The amount of motion, however, is much less, and was measured as about 0".07 in pa 103°. Evidently the two stars do not form a physical pair.
G273-081: No color estimate available: image off the edge of the red plate.
G273-086, G273-088: These two stars may possibly form a wide common motion pair, although the measured motions are not precisely identical. Separation about 5'.1 in pa 101°. [added comment: modern astrometry shows that the motions are significantly different.]
G273-097: Suspected white dwarf.
G273-100: This star was noted as slightly bluish by both observers.
G273-109: This star was noted as slightly bluish.
G273-114, G273-115: These for the common proper motion pair LDS 2995; separation about 17" in pa 241°.
G273-154: Luyten reports a companion of magnitude 19.5, separation 35" in pa 34°. The companion is LP 763-15; the two stars form the pair LDS 3003.
G273-175: This star is the close pair ADS 17107 or Σ3046. The Lick "Index Catalogue of Visual Double Stars" gives the individual magnitudes as 9.0 and 9.5, separation 3".6 in pa 260°(1959). Both the separation and the position angle have been increasing slowly over the past century.
G273-180, G273-181: These form the common proper motion pair LDS 831; separation about 31" in pa 142°.
G273-185, G273-186: These form the common proper motion pair LDS 830; separation about 20" in pa 114°.
G273-193: Additional references: BPM 68883, VM 528, and BD-20 6684.
G273-204: Luyten finds a close companion, which he designates LP 704-32. He reports a magnitude difference of about 0.7 mag, separation 2" in pa 72°.
G274-009: This is probably not LP 827-138, which Luyten lists near this position, at 1h18m18s -22°49' (1950). From a re-examination of the field on Lowell plates, it seems that the Luyten object may be a faint star lying 3'.8 distant from G274-9 in pa 334°. The images of this object are so near the plate limit that the motion cannot be confirmed, but the star is definitely quite red. Blue magnitude about 17.2.
G274-010: The images of this star are faint and difficult to measure; Luyten reports a somewhat larger position angle of 236°.
G274-014, G274-015: These two stars possibly form a common proper motion pair, although the measured position angles differ by about 7°. The difference may be due to the difficulty of measuring the faint, uncertain image of the companion, and the great magnitude difference between the two stars. The separation of the pair is about 57" in pa 148°. [added comment: modern astrometry confirms the common motion of the pair.]
G274-019: Luyten reports a faint companion to this star at a separation of 157" in pa 292°; magnitude 20.7. The companion is designated LP 883-265; the pair is also catalogued as LDS 2192.
G274-022: Luyten reports a faint companion to this star at a separation of 3".5 in pa 94°; magnitude 17.2. The companion is designated LP 883-278; the pair is also catalogued as LDS 2194.
G274-026: Refer to G269-155. Luyten reports this star to be a 6" pair, pa 340°, magnitudes 11.3 and 12.9. The fainter star is designated LP 827-203 in Luyten's lists.
G274-028, G274-029: Refer to G269-157, G269-158.
G274-039: This is the white dwarf suspect Ton S 217, called 'very blue' by E. Chavira (1958BOTT....2q..15C). Luyten's estimated color class is 'a'.
G274-046: This is undoubtedly LP 883-542, though there is a discrepancy in the Right Ascension, which Luyten gives as 1h17m12s.
G274-047: White dwarf suspect. Luyten's estimated color class is 'a'.
G274-058: This is Ton S 220, a suspected white dwarf. Luyten's estimated color class is 'a'. Luyten has also detected a faint companion to this star at 24" in pa 242°, magnitude 21+, color estimate 'm'. The faint star is designated LP 883-472; the pair has the number LDS 2209.
G274-061: This star has been published previously in one of the Lowell lists of very red stars under the designation GR 130.
G274-076: This is G272-062, but the CD number published previously was in error (CD-23 605). The correct number is CD-23 610.
G274-080: This star appears to be No. 682 in "A Finding List of Early-type Stars Near the South Galactic Pole" by A. Slettebak and R.K. Brundage (1971AJ.....76..338S). The authors class the spectrum as A0, though the images do not appear at all bluish on the Lowell plates.
G274-081, G274-082: Refer to G272-074, G272-075.
G274-091: This is not SB 718; the SB object lies about 5' to the east and 1'.2 to the south, and is evidently the same star as BPM 47333, for which Luyten obtains a a motion of 0".15 in pa 109°.
G274-095: White dwarf suspect. Luyten's estimated color class is 'a'.
G274-096: Luyten finds the star to be a close pair, which he designates LP 884-37 and LP 884-36, magnitudes 15.5 and 16.3, separation 3" in pa301°.
G274-099: The brightest star at the west edge of the finder chart is SB 740, for which Slettebak & Brundage report a spectral type of A7. The SB object show no definite motion on the Lowell plates.
G274-100: This is CD-32 709. Through an error the number is given as CD-33 709 in the Luyten list.
G274-103: A possible white dwarf suspect. Luyten's estimated color class is 'g'.
G274-107: A possible white dwarf suspect.
G274-126, G274-128: These two stars for the common proper motion pair LDS 61. The separation is about 42" in pa 163°.
G274-131: Luyten finds the star to a close pair, designated LP 828-45 and LP 828-46. Separation about 1", magnitudes 15.2 and 15.7, pa 90°. Both components are given an estimated color class of 'k-m'.
G274-137: White dwarf suspect. Luyten's estimated colors class is 'a'.
G274-138: Luyten finds the star to be a close pair, designated LTT 1075 and LTT 1076, also LP 828-60 and LP 828-61. Separation 3" in pa 69°, magnitudes 14.5 and 14.7. Both stars are classed as dM6 (cf 1985ApJS...59..197B).
G274-144: A possible white dwarf suspect. Luyten's estimated color class is 'f-g'.
G274-145, G274-146: These form the common proper motion pair LDS 67. Separation about 58" in pa 14°.
G274-147, G274-148: These form the common proper motion pair LDS 68. Separation about 57" in pa 257°.
G274-149: The CD number of CD-30 737 has been given as a reference by Luyten, but this appears to be an error; the motion star has no CD number. The bright star just to the east on the finder chart is -30 371.
G274-150: Suspected white dwarf. This is Ton S 238, classed by E. Chavira as 'very blue' (1958BOTT....2q..15C). Luyten's estimated color class is 'a'.
G274-153: Luyten reports a faint bluish companion to this star at a separation of 73" in pa 313°; he gives the magnitudes (photographic) as 14.4 and 16.0, and the estimated color classes as 'm' and 'a'. The brighter and redder star is LP 885-23; the blue companion is LP 885-22.
G275-001, G275-002: These two stars form a common proper motion pair with a separation of 150" in pa 48°. The brighter star is CD-23 17748.
G275-008: Suspected white dwarf. Luyten's estimated color class, reported in the LTT catalogue, is 'f'. The nearest field star on the identification chart, about 80" north-preceding, has a fairly large annual motion of about 0".18 in pa 160°. Magnitude on the Lowell blue plates about 14.0, estimated color +2.
G275-011: The is LP 877-70. Luyten finds a companion of photographic magnitude 18.0, which he designates LP 877-71. Separation 50" in pa 25°; Luyten's estimated color class for the faint star is 'm'.
G275-018: This is LP 985-106. The position angle of 150° published in the LTT catalogue appears to be a misprint.
G275-022: Suspected white dwarf. Luyten's estimated color class is 'k'.
G275-026: This is LTT 9453, also LP 933-79. The position angle of 296°reported in the LTT catalogue is an error; the correct position angle is about 54°.
G275-054: The second brightest star in the identification chart, 3'.4 east of G275-54, shows a measureable motion of about 0".14 annually in pa 205°. From the definite difference in motion and position angle, the two stars do not appear to form a common motion pair.
G275-057: Suspected white dwarf. The proper motion of the star is somewhat uncertain, owing to the very weak first-epoch plates images.
G275-062: This is BD-22 6144. Luyten reports a proper motion companion of magnitude 21.0, which he designates LP 878-51; separation 8" in pa 85°.
G275-073, G275-074: These two stars form a common proper motion pair with a separation of about 85" in pa 36°.
G275-075: This is the primary of Luyten's pair LDS 2291; the two stars are also listed as LP 878-5 and LP 878-6. Separation according to Luyten is 85" in pa 62°. The companion, claimed to be magnitude 16.8, could not be confirmed on Lowell plates.
G275-076: This is LTT 9637, but the reported CD number should be CD-30 19633 instead of CD-20 19633.
G275-090, G275-092: These two stars form a common proper motion pair with a separation of about 95" in pa 153°.
G275-101, G275-102: These two stars form a common proper motion pair with a separation of about 13" in pa 146°.
G275-108: This appears to BPM 68754, but the reported BPM motion is only 0".093.
G275-116: Suspected white dwarf. Luyten's estimated color class is 'a'.
G275-120: The reality of the motion is uncertain, owing to the very indistinct first-epoch plate image. [added comment: modern astrometry shows the motion to be near zero.]
G275-121: This star is a close pair, LDS 826 or LP 936-12 and LP 936-13. Luyten gives the individual magnitudes as 13.7 and 15.4, separation 7" in pa 1°. The primary is identified as a white dwarf of type DA (1952ApJ...116..283L).
G275-123: A color estimate of +1 was published previously (cf G266-003), but the star appears much redder on the G275 plates. Luyten's estimated color class is 'k'.
G275-126: This is identified as CD-31 19507 by Luyten, but that star shows no certain motion on Lowell plates. The correct CD number for the motion star is CD-30 19737.
G275-129: This is LTT 9788, but the CD number (CD-33 16752) given in the LTT catalogue is a misprint, and should be corrected to CD-33 16762.