CE 315: A New Interacting Double‐Degenerate Binary Star
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/552/i=2/a=679/pdf
Reference21 articles.
1. Double Degenerates among DA white dwarfs
2. In Search of the Progenitors of Type IA Supernovae
3. G61 - 29, a Helium Emission-Line Star
4. Ultrashort-Period Binaries. II. HZ 29 (=AM CVn): a Double-White Semidetached Postcataclysmic Nova?
5. Limits on the space density of double degenerates as type IA supernova progenitors
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