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## (from tabmap V5.8 (2012-11-24)) 2013-05-18T23:00:32
#---------------------------------------------------------------------------
#-- III/76A Luminous Stars in the Northern Milky Way (LS) (Hardorp+ 1959-1965)
#--------------------------------------------------------------------------
#---Table: III/76A/notes.dat Remarks originally in volumes II, IV and VI. (167 records)
# LS A7 --- *LS number, as in the file ls.dat
# Vol I1 --- *[1/6] Volume number, as in the file ls.dat
# Text A71 --- Text of note
#Note on LS, Vol:
# Columns are repeated when the note requires several lines.
#-------------------------------------------------------------------------------
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|V|
|o|
LS |l|Text
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+40 1|2|May be B7 II.
+39 47|2|May be cA.
+39 55|2|ADS 14314AB. The published delta m (Aitken, A New General Catalogue
+39 55|2|of Double Stars Within 120 deg of the North Pole) is so large that
+39 55|2|the observed spectrum must actually be entirely that of the primary.
+39 55|2|The primary is said to be composite in the Henry Draper Catalogue,
+39 55|2|and for this reason the star is given two HD numbers, HD 198287/8.
+39 55|2|The spectrum does not appear composite on our plates, and was charac-
+39 55|2|terized by Hynek (Perkins Contribution 1, No. 10, 1938) as one simu-
+39 55|2|lating compositeness because of high luminosity. This conclusion is
+39 55|2|almost certainly correct.
+38 17|2|May be B6 Ia.
+38 83|2|May be B7 Ib.
+37 35|2|May be B8 II.
+37 72|2|May be B7 Ir.
+36 8|2|May be B7 II.
+36 11|2|May be cA.
+36 86|2|ADS 14724A.
+35 33|2|ADS 13374A.
+35 61|2|May be B9 II.
+35 73|2|May be cA.
+34 12|2|May be B8 Ib.
+32 15|2|ADS 13335A.
+31 1|2|H-beta in emission.
+31 15|2|The type given here is purely descriptive; among the grounds for
+31 15|2|doubting it is the fact that the spectrum shows no reddening despite
+31 15|2|its low Galactic latitude. On the plate covering its position, an
+31 15|2|absorption feature which may be H-gamma is strong, while all other
+31 15|2|features, including the Balmer discontinuity, are at the limit of
+31 15|2|visiblity.
+30 17|2|May be B7 II.
+30 37|2|HR 8084.
+29 2|2|May be cA.
+29 5|2|P Cyg type. Strong H-alpha emission.
+29 6|2|Similar to AG Peg.
+29 22|2|May be cA.
+28 2|2|May be cA.
+24 26|2|B7 IV(e), Osawa, Ap. J. 130, 159, 1959.
+22 2|2|May be B8 Ib.
+22 3|2|ADS 12287AB.
+22 6|2|BDS 9287A.
+21 7|2|May be cA.
+17 3|2|ADS 11884A.
+16 4|2|Nucleus of planetary nebula No. 220 in Vorontsov-Velyaminov's catalogue
+16 4|2|(Gaseous Nebulae and New Stars, p. 563 ff. Moscow-Leningrad: Soviet
+16 4|2|Academy of Sciences, 1948).
+16 9|2|Perhaps B7 IIle.
+15 7|6|Weak ultraviolet.
+13 2|2|May be cA.
+13 9|6|Abnormal Balmer decrement.
+13 10|2|May be B6 Iab.
+11 2|2|ADS 12000AB.
+11 2|4|Flat continuum.
+11 3|6|K-line possibly present.
+11 5|2|Only one absorption spectrum is clearly identifiable in this overlap,
+11 5|2|and is assumed to belong to Aitken's component A.
+11 7|6|Weak ultraviolet.
+11 9|6|Ultraviolet also considered weak in this star.
+11 12|6|HR 2370, ADS 5153AB.
+10 2|4|Flat continuum.
+10 8|6|Nebulosity surrounds the star.
+09 3|4|May be composite.
+09 13|6|Precedes BD+09 1332 by only a few seconds of arc.
+09 14|6|ADS 5322AB, also S Mon; the slit classification is presumably for
+09 14|6|component A.
+09 15|6|ADS 5327AB.
+08 2|4|May be A0 I-II.
+08 3|6|May be composite.
+08 8|6|Probably not a true Wolf-Rayet, since Hiltner (Ap.J. Suppl. 2, No. 24,
+08 8|6|1956) refers to this star merely as showing high-excitation emission
+08 8|6|superposed on about an O9 spectrum.
+08 11|6|K-line present.
+08 12|6|Nebulosity surrounds the star.
+07 2|4|May be composite.
+07 7|6|K-line and perhaps 4026 present.
+06 1|6|Appears to be composite.
+06 2|6|K-line may be present.
+06 2|4|Very flat continuum.
+06 5|4|Flat continuum.
+06 6|4|G band possibly visible.
+05 3|4|Rather flat continuum.
+05 6|4|May be composite.
+05 13|6|Probably a double star.
+05 20|6|H-epsilon somewhat enhanced.
+05 21|6|K-line may be present; ultraviolet weak; composite?
+05 25|6|May be composite.
+04 1|4|Weak or variable K-line?
+04 8|6|May be composite.
+04 16|6|Helium I lines appear to be visible.
+04 35|6|K-line may be present.
+03 6|6|May be composite.
+03 12|4|May be composite.
+02 13|6|The small angular separation of this binary star assures that the pub-
+02 13|6|lished spectral type of B0 III:p pertains to the combined light of the
+02 13|6|system.
+02 14|6|Possibly composite.
+02 16|6|K-line may be present.
+01 5|4|May be composite.
+01 8|4|May be composite.
+01 10|4|May be composite.
+00 1|6|AGK2 asumes Aitken's position angle for AC is 180 degrees in error and
+00 1|6|calls this star component C; this seems true on a blue plate, but our
+00 1|6|red (H-alpha) plate supports Aitken.
+00 3|4|Flat continuum.
+00 5|4|Classified only from H-alpha plates.
+00 10|4|May be B8 II.
+00 21|4|Flat continuum.
-00 5|4|May be B7 II.
-00 7|6|May be composite.
-00 15|4|K-line visible?
-00 20|4|Composite?
-01 1|6|ADS 4141AB.
-01 16|6|May be B7 III.
-01 18|4|May be composite.
-02 1|6|ADS 4241ABC; a published spectral type of O9.5 V exists.
-02 3|4|K-line may be variable on our plates.
-02 6|4|May be B8 II-III.
-02 10|6|The published spectral type of B0.5 IV (2) must refer to the combined
-02 10|6|light of both components, in view of their small angular separation.
-02 14|4|May be composite.
-02 28|4|May be B8 II-III.
-03 9|4|Roberts 90.
-03 13|6|A spectral type of O9 V has been published for what is presumably
-03 13|6|component A.
-03 19|6|Flat continuum.
-04 8|4|May be composite.
-04 14|4|Roberts 89.
-04 24|6|May be B7 II-III.
-04 33|4|Roberts 91.
-05 1|6|May be double.
-05 12|6|K-line probably present.
-05 30|4|Composite?
-06 1|6|Nebulosity surrounds this star.
-06 7|4|Roberts 88.
-06 11|4|K-line present?
-06 29|4|K-line present?
-07 3|4|Composite?
-07 17|4|Composite?
-07 18|4|May be B7 II-III.
-07 24|4|May be B8 II-III.
-07 31|4|Flat continuum.
-08 27|4|K-line visible?
-08 29|4|K-line visible?
-09 7|6|Ultraviolet continuum weak.
-09 10|4|May be B7 II.
-09 11|4|Lambda 4686 emission?
-09 29|4|K-line visible?
-10 11|4|ADS 11414A; component B may be A- type.
-10 15|4|May be B7 II-III.
-10 16|4|May be B7 II.
-10 18|4|Composite?
-10 24|4|ADS 11670AB.
-10 29|4|Flat continuum.
-11 14|4|Roberts 85.
-11 15|4|Spectral appearance differs considerably between two plates; may be
-11 15|4|less luminous than OB-.
-11 20|4|Of?
-11 33|4|May be B7 II.
-12 5|4|The published spectral type is taken form Hiltner, but does not check
-12 5|4|with the star's appearance on our plates.
-12 56|4|May be composite.
-12 59|4|Classified only from an H-alpha plate.
-13 16|4|Close pair, both OB stars, originally classified as one star. The
-13 16|4|magnitude refers to the combined light.
-13 40|4|Roberts 86.
-13 71|4|May be composite.
-14 56|4|Roberts 87.
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