J/MNRAS/491/5489  Semi-detached double-lined eclipsing binaries   (Malkov, 2020)

Catalogue of semi-detached double-lined eclipsing binaries. Malkov O. <Mon. Not. R. Astron. Soc. 491, 5489 (2020)> =2020MNRAS.491.5489M 2020MNRAS.491.5489M (SIMBAD/NED BibCode)
ADC_Keywords: Binaries, eclipsing ; Stars, masses ; Stars, diameters ; Effective temperatures Keywords: binaries: close - binaries: eclipsing - stars: evolution Abstract: Semidetached eclipsing systems provide a unique opportunity to derive the basic properties of interacting binaries. The goal of this work is to collect and to make use of data on semidetached systems with available light and radial velocity curve solutions. I have compiled the most comprehensive list to date, of 119 semidetached double-lined eclipsing binaries, containing the orbital parameters and physical parameters of the components. I consider the classification of semidetached binaries and discuss gaps between various classes in the Hertzspung-Russell diagram. I list systems with component parameters that are inverted and briefly discuss their evolutionary state. Description: I have compiled a list of SD double-lined eclipsing binary (SD DLEB) systems with reliable parameters obtained from light-curves and radial velocity curves. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 171 119 Semi-detached double-lined eclipsing binaries -------------------------------------------------------------------------------- See also: V/115 : Semi-detached eclipsing binaries (Surkova+, 2004) J/other/A+AT/23.213 : Catalog of massive close binaries (Polushina, 2004) J/A+A/417/263 : Catalogue of Algol type binary stars (Budding+, 2004) J/MNRAS/373/435 : Angular momentum evolution of Algol binaries (Ibanoglu+, 2006) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- GCVS GCVS name 10- 21 F12.8 d Per Orbital period 23- 37 A15 --- SpType Spectral type 38- 44 F7.3 Msun M1 Primary mass (1) 46- 50 F5.3 Msun e_M1 ? Primary mass error 52- 57 F6.3 Msun M2 Secondary mass (1) 59- 63 F5.3 Msun e_M2 ? Secondary mass error 65- 70 F6.3 Rsun R1 Primary radius (1) 72- 76 F5.3 Rsun e_R1 ? Primary radius error 78- 83 F6.3 Rsun R2 Secondary radius (1) 85- 89 F5.3 Rsun e_R2 ? Secondary radius error 91- 95 I5 K T1 Primary effective temperature (1) 97-100 I4 K e_T1 ? Primary effective temperature error 102-106 I5 K T2 Secondary effective temperature (1) 108-111 I4 K e_T2 ? Secondary effective temperature error 113-118 F6.3 [Lsun] logL1 Primary log(Lbol) (1) 120-124 F5.3 [Lsun] e_logL1 ? Primary log(Lbol) error 126-131 F6.3 [Lsun] logL2 Secondary log(Lbol) (1) 133-137 F5.3 [Lsun] e_logL2 ? Secondary log(Lbol) error 139-144 F6.3 arcsec a Orbit semi-major axis 146-151 F6.3 arcsec e_a ? Orbit semi-major axis error 153-171 A19 --- BibCode Reference Bibcode -------------------------------------------------------------------------------- Note (1): Index '1' always corresponds to hotter component. -------------------------------------------------------------------------------- Acknowledgements: Oleg Malkov, malkov(at)inasan.ru
(End) Oleg Malkov [INASAN], Patricia Vannier [CDS] 13-Jan-2020
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