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Hydrodynamic studies of oxygen, neon, and magnesium novaeResults are presented from recent theoretical studies that have examined the properties of nova outbursts on ONeMg white dwarfs. These outbursts are much more violent and occur much more frequently than outbursts on CO white dwarfs. Hydrodynamic simulations of both kinds of outbursts are in excellent agreement with the observations.
Document ID
19880048394
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Starrfield, Sumner
(Los Alamos National Laboratory, NM; Joint Institute for Laboratory Astrophysics, Boulder CO, United States)
Sparks, W. M.
(Los Alamos National Laboratory NM, United States)
Truran, J. W.
(Illinois, University Urbana, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1987
Subject Category
Astrophysics
Meeting Information
Meeting: Stellar pulsation
Location: Los Alamos, NM
Country: United States
Start Date: August 11, 1986
End Date: August 15, 1986
Accession Number
88A35621
Funding Number(s)
CONTRACT_GRANT: NSF AST-83-14415
CONTRACT_GRANT: NAG5-481
CONTRACT_GRANT: NSF AST-85-16173
CONTRACT_GRANT: NSF AST-83-14788
Distribution Limits
Public
Copyright
Other

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