V/35 Catalogue of nearby stars, Revised version 2 (Gliese+ 1979) ================================================================================ Catalogue of nearby stars and nearby star data published 1969-78 Gliese W., Jahreiss H. =1979A&AS...38..423G =2015yCat.5035....0G ================================================================================ ADC_Keywords: Stars, nearby ; Proper motions ; Radial velocities ; Spectral types ; Magnitudes, absolute ; Parallaxes, spectroscopic ; Parallaxes, trigonometric ; Space velocities Keywords: Nearby stars ; star: catalogue ; stellar parallaxes Description: From trigonometric parallaxes and from spectroscopic and photometric data published since 1969 and available before January 1979, 3 lists have been compiled: (1) Stars of the second edition of the catalogue of nearby stars (V/1) (main.dat) with revised parameters published in table 3 of the paper; it includes also additional faint components (table 4) (2) Additional stars with parallaxes {pi}>=0.045arcsec (nearer than 22pc) (suppl.dat), contains 294 new objects numbered between 1001 and 1294; it was published as the Table 1 of the paper. The identifications of these new systems are given in the file "supplid.dat" (3) Suspected nearby stars: 159 objects with uncertain distance data, published as the Table 2 of the papers, numbered 2001 to 2159 (suspect.dat) File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file main.dat 132 1899 Stars of Edition 2 suppl.dat 130 333 Supplement of stars with distance <=22pc (table 1) supplid.dat 116 333 Identifications of the supplement stars (table 1) suspect.dat 139 172 Stars suspected to be within 22pc (table 2) -------------------------------------------------------------------------------- J See also: V/32 : Stars within 25pc of the Sun (Woolley+ 1970) Byte-by-byte Description of file: main.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 F5.1 --- Gl [1/915] Star number (1) 6 A1 --- m_Gl [ABCD] Multiplicity index 7 A1 --- f_Gl [*] The asterisk indicates a star beyond 22pc. 8- 19 A12 --- Name Common name of the star 20- 25 I6 --- HD ? Henry Draper (III/135) identification 26- 27 I2 h RAh Right Ascension B1950 (hours), Ep=B1950 28- 29 I2 min RAm Right Ascension B1950 (minutes), Ep=B1950 30- 31 I2 s RAs Right Ascension B1950 (seconds), Ep=B1950 32 A1 --- DE- Declination B1950 (sign), Ep=B1950 33- 34 I2 deg DEd Declination B1950 (degrees), Ep=B1950 36- 38 I3 0.1arcmin DEdm Declination B1950 (deci-minutes), Ep=B1950 40- 44 I5 0.1ms/yr pmRA Proper motion along RA 45- 49 I5 mas/yr pmDE Proper motion along Declination 50- 53 I4 km/s RV ? Radial velocity 55 A1 --- q_RV [A-E*] Quality of radial velocity, A=best (G2) 56 A1 --- Lw [3-7C] Wilson's luminosity class (3) 57- 59 A3 --- Sp Spectral temperature class (3) 60 A1 --- LC [1-9] MK luminosity classification (3) 61 A1 --- pec [1-9] Spectral peculiarity (3) 62 A1 --- Sj [J] for a joint spectral type (binary) 63 A1 --- Sr [CEGHKLMOW] Origin of the spectral type (4) 65- 68 I4 cmag Vmag ? V-band magnitude 69 A1 --- f_Vmag [PJ*] Vmag is Photographic (P), Joint (J) or reduced from non-standard system (*) 71- 73 I3 cmag B-V ? (B-V) color 74 A1 --- f_B-V [J] Joint color 75- 78 I4 cmag U-B ? (U-B) color 79 A1 --- f_U-B [J] Joint color 81- 83 I3 cmag R-I ? (R-I) color 84 A1 --- f_R-I [J] Joint color 86- 88 I3 mas pi.t ? Trigonometric parallax {pi}_t_ 90- 91 I2 mas e_pi.t ? Probable error on pi.t 93- 95 I3 dmag Mt ? Trigonometrically determined Absolute magnitude 96 A1 --- q_Mt [B-FP] Quality pf Mt (G1) 98-100 I3 mas pi.s ? Spectroscopic parallax {pi}_s_ 101 A1 --- f_pi.s [U] Uncertain pi.s 103-105 I3 mas pi.p ? Photometric parallax {pi}_p_ 106 A1 --- f_pi.p [U] Uncertain pi.p 108-110 I3 mas pi.r ? Resulting parallax {pi}_r_ 112-113 I2 mas e_pi.r ? Probable error on pi.r 115-118 I4 cmag Mres ? Resulting absolute magnitude M_res_ 119 A1 --- f_Mres [P] Photographic absolute magnitude 120 A1 --- q_Mres [A-F] Quality of Mres (G1) 121-124 I4 km/s Uvel ? U-component of spatial velocity (6) 125-128 I4 km/s Vvel ? V-component of spatial velocity (6) 129-132 I4 km/s Wvel ? W-component of spatial velocity (6) -------------------------------------------------------------------------------- Note (1): the numbers of the first edition have a ".0" fraction; new stars are added in order of increasing RA Note (3): Spectral type components are: * Wilson's luminosity class, which is is coded as 3=g(giant) 4=sg(subgiant) 5=d(dwarf) 6=sd(subdwarf) 7=D(degenerate) C=spectral class is a color estimate by Luyten or Giclas * the temperature class (no decimal point in the subclass, e.g. "M55" should be understood as "M5.5") * the MK luminosity class is a number meaning 1=II(giant) 2=III(giant), 3=III-IV, 4=IV(subgiant), 5=IV-V, 6=IV,V 7=V, 8=V-VI, 8=VI(subdwarf) * the peculiarities are coded as 1=p(peculiar), 2=e(emission), 4=m(metallic), 5=s(sharp lines), 6=ss(very sharp lines), 7=ep(emission+peculiar), 8=n(nebulous lines), 9=wk(weak-line) Note (4): references of the spectral type: C = Cape Observatory E = Eggen (data for white dwarfs) G = Giclas (Lowell Proper Motion survey) H = Harvard (HD spectra) K = Kuiper (many late-type stars) L = Luyten (mostly color classes f, g, k, m given here as F, G, K, M with a "C" preceding) M = McCormick (mostly red dwarfs on Vyssotsky's program) O = MK classifications on objective prism plates W = Mount Wilson (mainly from the "General Catalog of Stellar Radial Velocities, see III/21) Note (6): the components of the spatial velocity a positive toward * the galactic center (U) * the galactic rotation (V) * the North galactic pole (W) -------------------------------------------------------------------------------- Byte-by-byte Description of file: suppl.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 6 I4 --- GJ [1001/1294] Star number 7- 8 A2 --- m_GJ [AB C-] Multiplicity index 10- 11 I2 h RAh Right Ascension B1950 (hours), Ep=B1950 13- 14 I2 min RAm Right Ascension B1950 (minutes), Ep=B1950 16- 17 I2 s RAs Right Ascension B1950 (seconds), Ep=B1950 20 A1 --- DE- Declination B1950 (sign), Ep=B1950 21- 22 I2 deg DEd Declination B1950 (degrees), Ep=B1950 24- 27 F4.1 arcmin DEm Declination B1950 (deci-minutes), Ep=B1950 30 A1 --- ch [GR*] Chart origin (G4) 33- 36 F4.2 arcsec/yr pm ? Total proper motion 38- 40 I3 deg pmPA [0/360]? Proper motion position angle 43- 46 I4 km/s RV ? Radial velocity 48 A1 --- q_RV [A-E*] Quality of radial velocity, A=best (G2) 49 A1 --- r_RV [RGTW] Origin of the radial velocity (2) 52- 58 A7 --- SpT MK Spectral type 61- 65 F5.2 mag Vmag ? V-band magnitude 66- 67 A2 --- n_Vmag [: PJ*] Vmag is not in standard system (G5) 69- 73 F5.2 mag B-V ? (B-V) color 74- 75 A2 --- f_B-V [: *J] (B-V) flag (G5) 77- 81 F5.2 mag U-B ? (U-B) color 82 A1 --- f_U-B [:*JC] (U-B) flag (G5) 85- 89 F5.2 mag R-I ? (R-I) color 90 A1 --- f_R-I [:*J] (R-I) flag (G5) 93- 95 I3 mas pi.t ? Trigonometric parallax {pi}_t_ 96 A1 --- --- [~] 97- 98 I2 mas e_pi.t ? Probable error on pi.t 100-107 A8 --- r_pi.t Reference(s) of parallaxes 109-113 F5.2 mag Mt ? Absolute magnitude from trigo. parallax 115 A1 --- q_Mt [A-FP] Quality of Mt, A=best (G1) 118-120 I3 mas pi.s ? Specroscopic or photometric parallax 123-126 F4.1 mag Ms ? Absolute magnitude from pi.s 127 A1 --- u_Ms Uncertainty flag on Ms 128-130 A3 --- r_Ms ? Source of Ms (G3) -------------------------------------------------------------------------------- Note (2): Origin of the radial velocity: R = Rodgers & Eggen 1974PASP...86..742R G = Greenstein & Trimble 1967ApJ...149..283G T = Trimble & Greenstein 1972ApJ...177..441T W = Wegner 1974MNRAS.166..271W -------------------------------------------------------------------------------- Byte-by-byte Description of file: supplid.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 6 I4 --- GJ [1001/1294] Star number 7- 8 A2 --- m_GJ [AB C-] Multiplicity index 12- 15 I4 --- LHS ? Identifier in LHS (Luyten 1979, see Cat. I/87) 16 A1 --- m_LHS [A] Additional star in LHS 19- 23 I5 --- LTT ? Identifier in Luyten's Two Tenths (Minneapolis) 27- 30 I4 --- LFT ? Identifier in Luyten's Five Tenths (Minneapolis) 34- 41 A8 --- G Identifier in Giclas lists (I/79, I/112) 45- 47 I3 --- EgGr ? Identifier in Eggen/Greenstein lists 51- 54 A4 --- V/U Identifier in Vyssotsky's or Upgren's lists 58- 67 A10 --- DM Durchmusterung identifier: BD({delta}>-22) or CD 71- 78 A8 --- CPD Cape Photographic Durchmusterung (I/108) 82- 87 I6 --- HD ? Henry Draper Identifier (III/135) 91- 95 I5 --- GC ? General Catalog (B.Boss, I/113) 100-116 A17 --- OName Other identifications (comma-separated list) -------------------------------------------------------------------------------- Byte-by-byte Description of file: suspect.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 6 I4 --- GJ [2001/2159] Star number 7- 8 A2 --- m_GJ [AB C-] Multiplicity index 10- 11 I2 h RAh Right Ascension B1950 (hours), Ep=B1950 13- 14 I2 min RAm Right Ascension B1950 (minutes), Ep=B1950 16- 17 I2 s RAs Right Ascension B1950 (seconds), Ep=B1950 20 A1 --- DE- Declination B1950 (sign), Ep=B1950 21- 22 I2 deg DEd Declination B1950 (degrees), Ep=B1950 24- 27 F4.1 arcmin DEm Declination B1950 (deci-minutes), Ep=B1950 30 A1 --- ch [EGRLS*] Chart origin (G4) 32 A1 --- l_pm [<] Limit flag on proper motio n 33- 36 F4.2 arcsec/yr pm ? Total proper motion 38- 40 I3 deg pmPA [0/360]? Proper motion position angle 51- 58 A8 --- SpT MK Spectral type 61- 65 F5.2 mag Vmag ? V-band magnitude 66- 67 A2 --- n_Vmag [: PJ*] Vmag is not in standard system (G5) 69- 73 F5.2 mag B-V ? (B-V) color 74- 75 A2 --- f_B-V [: *J] (B-V) flag (G5) 77- 81 F5.2 mag U-B ? (U-B) color 82 A1 --- f_U-B [:*JC] (U-B) flag (G5) 85- 89 F5.2 mag R-I ? (R-I) color 90 A1 --- f_R-I [:*J] (R-I) flag (G5) 93- 96 F4.1 mag Ms ? Absolute magnitude from pi.s 97 A1 --- u_Ms [:P] uncertain Ms (:), or photographic (P) 98 A1 --- r_Ms [EGSd*] Source of Ms: Eggen, Greenstein, or Stephenson; d if strar assumed to be a dwarf, and * refers to a note in the original paper 101-104 F4.1 mag m-M ? Distance modulus 105 A1 --- u_m-M Uncertainty flag on m-M 108-139 A32 --- Names Comma-separated name(s) of the star -------------------------------------------------------------------------------- Global Notes: Note (G1): Qualities of the absolute magnitude (p.e. means "probable error"): A = p.e.<=0.08mag B = 0.09mag<=p.e.<=0.15mag C = 0.16mag<=p.e.<=0.25mag D = 0.26mag<=p.e.<=0.35mag E = 0.36mag<=p.e.<=0.50mag; from Eggen F = p.e.>0.5mag P = photographic absolute magnitude is given * = discussion in the notes of the printed table Note (G2): The qualities are (p.e. means "probable error"): A = well determined, p.e.<=0.9km/s B = good, 0.9km/s10km/s, to be ignored. * = inaccurate, velocity of a white dwarf Note (G3): Sources of absolute magnitude: E1 = Eggen 1974PASP...86..697E E2 = Eggen 1976ApJS...30..351E, 1976ApJ...204..101E G1 = Greenstein 1976AJ.....81..323G G2 = Greenstein et al. 1977ApJ...218L..21G M = McCormick: Vyssotsky et al. 1943ApJ....97..381V, 1946ApJ...104..234V, 1952ApJ...116..117V, 1956AJ.....61..201V RE = Rodgers & Eggen 1974PASP...86..742R Note (G4): finding charts are in: E = Eggen G = Giclas (details in Table 5 of original paper) L = Luyten (1949ApJ...109..528L) R = Rodgers & Eggen (1974PASP...86..742R) S = Sanduleak (1976AJ.....81..350S) * = in the notes of paper, Note (G5): the colors are in principle in the Johnson system (UBV) and Kron (RI). The flags are: : = uncertain value P = photographic magnitude J = joint photometry (color of merged components) * = reduced from non-standard system C = (U-B) in Cape system -------------------------------------------------------------------------------- History: * The tables were originally forwarded by the authors to CDS in 1979 (see the paper by the authors in the "Bulletin d'Information du CDS", 1979BICDS..16...92G) * The documentation was added in 2015. ================================================================================ (End) Francois Ochsenbein [CDS] 17-Dec-2015