A limit cycle model for long-term optical variations of V Sagittae: The second example of accretion wind evolution

Astrophysical Journal

Volumn 598, Issue 1 I, 2003, Pages 527-544

  Hachisu, Izumi ^a   Kato, Mariko ^b  

^a UNIVERSITY OF TOKYO   (Japan)

^b KEIO UNIVERSITY   (Japan)

Author keywords

Binaries: close; Novae, cataclysmic variables; Stars: individual (V Sagittae); Stars: winds, outflows; X rays: stars

Indexed keywords

EID: 0347527138     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/378848     Document Type: Article

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