Fundamental parameters, helium abundance and distance of X Persei

Monthly Notices of the Royal Astronomical Society

Volumn 286, Issue 3, 1997, Pages 549-557

  Lyubimkov, L S ^a   Rostopchin, S I ^a   Roche, P ^b   Tarasov, A E ^a  

^a CRIMEAN ASTROPHYSICAL OBSERVATORY   (Ukraine)

^b UNIVERSITY OF SUSSEX   (United Kingdom)

Author keywords

Circumstellar matter; Stars: abundances; Stars: emission line, Be; Stars: fundamental parameters; Stars: individual: X Per

Indexed keywords

ABSORPTION SPECTROSCOPY; STARS; THERMAL LOGGING;

BE-X-RAYS:BINARIES; BINARY SYSTEMS; CIRCUMSTELLAR MATTERS; HELIUM ABUNDANCE; SPECTRAL OBSERVATIONS; STAR: INDIVIDUAL: X PER; STARS ABUNDANCES; STARS: EMISSION-LINE BE; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:FUNDAMENTAL PARAMETERS;

LUMINANCE;

EID: 0000653858     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/286.3.549     Document Type: Article

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