A theoretical light-curve model for the recurrent nova V394 Coronae Australis

Astrophysical Journal

Volumn 540, Issue 1 PART 1, 2000, Pages 447-451

  Hachisu, Izumi ^a   Kato, Mariko ^b  

^a UNIVERSITY OF TOKYO   (Japan)

^b KEIO UNIVERSITY   (Japan)

Author keywords

Accretion, accretion disks; Binaries: close; Novae, cataclysmic variables; Stars: individual (V394 Coronae Australis)

Indexed keywords

EID: 0034260009     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/309338     Document Type: Article

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