5032A V/32A Stars within 25 pc of the Sun R V D R Woolley E A Epps M J Penston S B Pocock Royal Obs. Ann. 5 ??? ??? 1970 1970ROAn....5....1W V/70 : Nearby Stars 3, Preliminary (Gliese, Jahreiss 1991) Gliese, W. 1957, "Katalog der Sterne naher als 20 Parsek fuer 1950.0", Astron. Rechen-Inst. Heidelb., Mitt. A, Nr. 8 Jenkins, L.F. 1952, General Catalogue of Trigonometric Stellar Parallaxes (New Haven; Yale University Observatory) Jenkins, L.F. 1963, Supplement to the General Catalogue of Trigonometric Stellar Parallaxes (New Haven; Yale University Observatory) Wilson, R.E. 1953, General Catalogue of Stellar Radial Velocities, Publ. Carnegie Inst., Washington, No. 601 Stars, nearby This catalog was constructed at the Royal Greenwich Observatory in order to enlarge the Gliese (1957) compilation. It contains data on stars nearer than 25 pc that are not included in Gliese's catalog, plus additional information published since 1957 on stars in the Gliese catalog. The machine version contains essentially all information given in Table Ia of the published catalog, plus positional data, and most cross references to other catalogs given in Table IIa. The notes flags in Table Ia are not included because the notes are not machine-readable. Omitted from Table IIa are the finding-chart indicators (Lowell G numbers or notes references) and miscellaneous cross identifications to other names and catalog identifiers. Tables Ib and IIb, containing 21 systems originally included in Gliese's (1957) catalog but for which revised parallaxes have placed them farther than 25 pc are not included in the machine version. Data in the machine version are Gliese number (Newly added stars begin with 9001, but new parallaxes have removed 9419 and added 9849 and 9850; the Sun [first record] has number 0); component identifications for multiple systems; parallax; annual proper motions; radial velocity; (U,V,W) space velocities; box orbit parameters (omega, e, i); spectral type; UBV data; absolute visual magnitude; right ascension (B1950) declination, GCTP (Jenkins 1952, 1963); HD DM, GCRV (Wilson 1953) and other catalog identifiers; BS (= HR) (Hoffleit 1964) numbers; and remarks codes for SB, doubles, variables, etc. Please note that the first entry is for the Sun, and thus it lacks fields such as RA and Dec.

Woolley Sequence number Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- m_Woolley Component identification number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- plx Parallax number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. mas e_plx Probable error in plx "S" indicates spectroscopic parallax number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. mas n_plx Note:'8' if e_plx < 15%, '9' if e_plx < 10% number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- pmRA Proper motion in RA number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. s/yr pmDE Proper motion in Dec number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. arcsec/yr RVel Radial velocity number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. km/s n_RVel Note on RV J = combined components of binary V = variable velocity number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- U U component of space velocity (toward galactic centre) number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. km/s V V component of space velocity (toward galactic rotation) number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. km/s W W component of space velocity (toward North galactic pole) number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. km/s GCdist Galactocentric distance in units of Sun's distance from the center i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. 10-4 e Box orbit eccentricity number=1 see details in file "adc.doc" or in the original publication. --- i Box orbit angle (highest inclination of the orbit) number=1 see details in file "adc.doc" or in the original publication. 10-4rad LC_Code Luminosity class code 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- SpType Spectral type number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- r_SpType Coded source of spectral type 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- Mag Magnitude m(v) or m(pg) (see n_Mag) number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. mag n_Mag Magnitude code J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- B-V B-V color number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. mag U-B U-B color number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. mag Mv Absolute visual magnitude Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. mag RA1900h Hours RA, equinox B1900, epoch 1900.0 number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. h RA1900dm Minutes RA, equinox B1900, epoch 1900.0 number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. 0.1min DE1900- Sign Dec, equinox B1900, epoch 1900.0 number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- DE1900d Degrees Dec, equinox B1900, epoch 1900.0 number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. deg DE1900m Minutes Dec, equinox B1900, epoch 1900.0 number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. arcmin RAh Right Ascension B1950, epoch 1950 (hours) number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. h RAm Right Ascension B1950, epoch 1950 (minutes) number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. min RAs Right Ascension B1950, epoch 1950 (seconds) number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. s DE- Declination B1950, epoch 1950 (sign) number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- DEd Declination B1950, epoch 1950 (degrees) number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. deg DEdm Declination B1950, epoch 1950 (deci-minutes) number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. 0.1arcmin GCTP Gen. Cat. of Trigonometric Parallaxes <I/60> number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- HD Henry Draper Catalog (HD) number number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- DM Durchmusterung (BD, CD, or CP) number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- GCRV Gen. Cat. of Radial Velocities (GCRV) number number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- PM_Name Name from other proper-motion catalog number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- HR Bright Star = Harvard Revised catalog <V.50> number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- Vys Number in red dwarf lists of Vyssotsky number= Star sequence numbers less than 1000 are from Gliese (1957); new stars have a number > 9000; The Sun is #0 (and therefore lacks entries in fields such as the RA and Dec. number= "S" indicates spectroscopic parallax number= J = combined components of binary V = variable velocity number= i.e GCdist represents parsecs if the Sun distance is 10kpc. See also in file "adc.doc" number= 1 = I or c; 2 = II or c; 3 = III or g; 4 = IV or sg; 5 = V or d; 6 = VI or sd; 7 = D or wd. Intermediate classes have no codes, e.g. 4 is given for IV-V. number= 1 if MK; 2 if combined MK type for multiple system; 4 if combined non-MK; blank if non-MK. number= J = combined light for multiple system P = Mag indicates a photographic magnitude V = variable magnitude number= Visual magnitude is reported to 0.01 mag if both probable error of parallax < 10% and V is given to 0.01 mag. --- Remark1 First remark code number=2 the codes are 2 = spectroscopic binary 3 = spectroscopic triple 4 = unresolved double, unknown nature 5 = UV Ceti flare star 6 = eclipsing binary 7 = semi-regular variable 8 = astrometric binary 9 = planetary nebula --- Remark2 Second remark code number=2 the codes are 2 = spectroscopic binary 3 = spectroscopic triple 4 = unresolved double, unknown nature 5 = UV Ceti flare star 6 = eclipsing binary 7 = semi-regular variable 8 = astrometric binary 9 = planetary nebula --- adc.docOriginal Documentation by Wayne H. Warren Jr. Francois Ochsenbein CDS James Gass SSDOO/ADC 1997Jul21 UNKNOWN UNKNOWN * 19-Jul-1994: The file has been reformatted at CDS from the CD-ROM version "Selected Astronomical Catalogues Vol.1" with addition of decimal points when required (blank numbers in the decimal part) and conversion of RVel and Mag codes. * The 1950 declination of Gliese 157B (record #350) was corrected. * 21-Jul-1997: This document was brought up to current CDS/ADC standards. [J. Gass, ADC] V_32A.xml