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1986ApJ...311..163S - Astrophys. J., 311, 163-171 (1986/December-0)
Do novae hibernate during most of the millennia between eruptions ? Links between dwarf and classical novae, and implications for the spacedensities and evolution of cataclysmic binaries.
SHARA M.M., LIVIO M., MOFFAT A.F.J. and ORIO M.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Stars: Dwarf Novae - Stars: Evolution - Stars: Mass Loss - Stars: Novae - Stars: Stellar Statistics
Simbad objects: 18
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