Determining the spectroscopic mass ratio in interacting binaries: Application to X-Ray Nova Sco 1994

Monthly Notices of the Royal Astronomical Society

Volumn 339, Issue 4, 2003, Pages 1031-1040

  Shahbaz, T ^a  

^a Instituto de Astrofísica de Canar Ias   (Spain)

Author keywords

Binaries: Close; Stars: Fundamental parameters; Stars: Individual: X ray nova sco 1994 (gro j1655 40); X rays: Stars

Indexed keywords

BINARIES: CLOSE; LIMB DARKENING; MASS RATIO; SECONDARY STARS; SPECTRA'S; STAR: INDIVIDUAL: X-RAY NOVA SCO 1994 (GRO J1655 - 40); STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:FUNDAMENTAL PARAMETERS; SYNTHETIC SPECTRA; X-RAY:STARS;

STARS;

EID: 0142073861     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06258.x     Document Type: Article

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