On the Relative Rates of Decay of the Optical and Soft X-Ray Fluxes in Dwarf Nova Outbursts
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference16 articles.
1. Cannizzo, J. K. 1993a, in Accretion Disks in Compact Stellar Systems, ed. J. C. Wheeler (Singapore: World Scientific), 6
2. The Accretion Disk Limit Cycle Model: Toward an Understanding of the Long-Term Behavior of SS Cygni
3. The Accretion Disk Limit Cycle Instability in Black Hole X-Ray Binaries
4. On the long-term behavior of SS Cygni
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2. TheV−EUV Delay for Dwarf Nova Outbursts: A Case Study for VW Hydri, U Geminorum, and SS Cygni;The Astrophysical Journal;2001-08
3. A Hot Inner Disk during the Quiescent State of Soft X‐Ray Transients?;Publications of the Astronomical Society of the Pacific;2000-10
4. On the Role of Irradiation and Evaporation in Strongly Irradiated Accretion Disks in the Black Hole X-Ray Binaries: Toward an Understanding of FRED[CLC]s[/CLC] and Secondary Maxima;The Astrophysical Journal;2000-05-01
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