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Volumn 313, Issue 2, 2000, Pages 383-391
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A mystery solved: The mass ratio of the dwarf nova EM Cygni
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Author keywords
Accretion, accretion discs; Binaries: spectroscopic; Novae, cataclysmic variables; Stars: individual: EM Cyg; Techniques: radial velocities
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Indexed keywords
SPECTROSCOPIC ANALYSIS;
VELOCITY;
WHITE DWARFS;
ACCRETION: ACCRETION DISKS;
BINARIES: SPECTROSCOPIC;
DWARF NOVAE;
MASS RATIO;
MEASUREMENTS OF;
NOVAE CATACLYSMIC VARIABLES;
SPECTRA'S;
STAR: INDIVIDUAL: EM CYG;
STARS: INDIVIDUAL: PROXIMA CENTAURI;
TECHNIQUES: RADIAL VELOCITIES;
MASS TRANSFER;
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EID: 0012468551
PISSN: 00358711
EISSN: None
Source Type: Journal
DOI: 10.1046/j.1365-8711.2000.03329.x Document Type: Article |
Times cited : (29)
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References (25)
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