The detection of A 3.5 hr period in the classical nova velorum 1999 (V382 Vel) and the long-term behavior of the nova light curve

Astronomical Journal

Volumn 131, Issue 5, 2006, Pages 2628-2633

  Balman, Şölen ^a,b   Retter, Alon ^c   Bos, Marc ^d  

^a MIDDLE EAST TECHNICAL UNIVERSITY   (Turkey)

^b EUROPEAN SPACE AGENCY   (Netherlands)

^c PENNSYLVANIA STATE UNIVERSITY   (United States)

^d Mount Molehill Observatory   (New Zealand)

Author keywords

Accretion, accretion disks; Binaries: close; Novae, cataclysmic variables; Stars: individual (V382 Velorum); White dwarfs

Indexed keywords

EID: 33745345284     PISSN: 00046256     EISSN: None     Source Type: Journal    
DOI: 10.1086/503161     Document Type: Article

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