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II/150A        Parameters of eclipsing binaries  (Brancewicz+, 1980)

A Catalogue of Parameters for Eclipsing Binaries Brancewicz H.K., Dworak T.Z. <Acta Astronomica 30, 501 (1980)> =1980AcA....30..501B
ADC_Keywords: Binaries, eclipsing Description: An iterative method has been used to compute the geometric and physical parameters of 1048 eclipsing binary stars. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file catalog.dat 130 1048 The catalogue
See also: II/139 : General Catalog of Variable Stars (GCVS), 4th Ed. (Kholopov+ 1988) V/46 : Classical (Evolved) Algol-Type Binary Candidates (Budding 1984) Byte-by-byte Description of file: catalog.dat
Bytes Format Units Label Explanations
1- 10 A10 --- Name Name of star 12 A1 --- Cester [*] * if the star is present in Cester's (1979, 1980) catalogue & first supplement 14- 24 F11.6 d Per Period in days 26- 29 I4 10-5arcsec Plx Parallax 31- 37 F7.2 solRad Sep Separation between the components in Solar radii 39- 45 F7.2 solRad R1 Radius of brighter component 47- 53 F7.2 solRad R2 Radius of fainter component 55- 57 I3 % RL1 Percent of filling up of Roche-lobe 59- 61 I3 % RL2 Percent of filling up of Roche-lobe 63- 71 F9.2 solLum L1 Absolute bolometric luminosity 73- 81 F9.2 solLum L2 Absolute bolometric luminosity 83- 87 I5 K T1 Effective temperature 89- 93 I5 K T2 Effective temperature 95- 99 F5.2 solMass M Sum of masses in solar units 101-104 F4.2 --- q Mass ratio q = M2/M1 106-110 F5.2 solMass M1 Mass of brighter component (solar masses) 112 A1 --- Class *[ABEW] Traditional Classification from GCVS (Kukarkin et al, cat. II/139) 114 A1 --- Kopal *[CDS] Kopal's geometrical classification 116-130 A15 --- Sp *Spectrum
Note on Class: See GCVS (cat. II/139), principal classes are: A = Algol type E = Eclipsing binary B = beta Lyr type W = W UMa type Note on Kopal: this class depends on Roche-lobe radii, as: C = Contact system (ex. W UMa) D = Detached system (ex. beta Lyr) S = Semi-detached system (ex. Algol = beta Per) Note on Sp: The colon denotes uncertain information, round brackets denote that the adopted spectrum for a fainter component was taken from Koch et al. (1970), and square brackets that the adopted spectrum was taken from Svechnikov (1969)
History: * The catalogue was keystroked at CDS in 1987 from the published table, which is of poor quality * 21-Jun-1996 (version A): following remarks by Eric Lefevre , a consistency check of the masses was performed and led to corrections to the following 14 stars: LR ARA RX ARI ZZ AUR AK AUR UZ CMI UW CAP V402 CEN NY CEP V388 CYG BO HER LX PER AW UMA RV VEL TT VEL * 29-Jun-1999: corrected NU SGR into UPS SGR (F. Ochsenbein) References: Cester B., et al.: 1979, Mem. Soc. Astron. Ital., 50, 551 =1979MmSAI..50..551C Cester B., et al.: 1980, Mem. Soc. Astron. Ital., 51, 197 =1980MmSAI..51..197C Koch, R.H., Plavec, M. and Wood, F.B.: 1970, "A catalogue of Graded Photometric studies of Close Binaries", Publ. Univ. Penn. Astr. Series, Volume X, Philadelphia Svechnikov, M.A.: 1969, Katalog orbitalnyich elementov, mass i svetimostei tesnyich dvoinyich zvezd, A.M.Gorky University of the Urals, Sverdlovsk.
(End) Joseph Florsch , Francois Ochsenbein [CDS] 21-Jun-1996
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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