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Volumn 382, Issue 1, 2002, Pages 124-129

Implications of the HST/FGS parallax of SS Cygni on the disc instability model

Author keywords

Accretion, accretion discs; Binaries: close; Novae, cataclysmic variables; Stars: individual: SS Cygni

Indexed keywords

GALAXIES; MASS TRANSFER; MATHEMATICAL MODELS; VISCOSITY;

EID: 0036187904     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20011627     Document Type: Article
Times cited : (33)

References (27)


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.