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Volumn 313, Issue 2, 2000, Pages 383-391

A mystery solved: The mass ratio of the dwarf nova EM Cygni

Author keywords

Accretion, accretion discs; Binaries: spectroscopic; Novae, cataclysmic variables; Stars: individual: EM Cyg; Techniques: radial velocities

Indexed keywords

SPECTROSCOPIC ANALYSIS; VELOCITY; WHITE DWARFS;

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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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.