Mapping the secondary star in QQ vulpeculae

Monthly Notices of the Royal Astronomical Society

Volumn 310, Issue 1, 1999, Pages 123-145

  Catalan M S ^a   Schwope, A D ^b   Smith, Robert Connon ^c  

^a KEELE UNIVERSITY   (United Kingdom)

^b ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^c UNIVERSITY OF SUSSEX   (United Kingdom)

Author keywords

Binaries: close; Novae, cataclysmic variables; Stars: fundamental parameters; Stars: imaging; Stars: Individual: QQ Vul; Stars: late type

Indexed keywords

ABSORPTION SPECTROSCOPY; MAGNESIUM COMPOUNDS; SODIUM COMPOUNDS; WHITE DWARFS;

BINARIES: CLOSE; NOVAE CATACLYSMIC VARIABLES; SECONDARY STARS; SPECTRA'S; STAR: INDIVIDUAL: QQ VUL; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:FUNDAMENTAL PARAMETERS; STARS:IMAGING; STARS:LATE TYPE; SURFACE MAP;

VELOCITY;

EID: 0000292221     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1999.02972.x     Document Type: Article

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