Models of Soft X-Ray Transients and Dwarf Novae
arXiv:astro-ph/9509003 · doi:10.1007/978-94-009-0325-8_118
Abstract
Models of Soft X--ray Transients are presented and compared with observations. The importance of inner advection--dominated flows in quiescent transient sources is discussed, as well as the problem of global stability of the standard outer accretion disc. A comparison is made with similar problems in dwarf nova models.
10 pages, 3 figures (available as uuencoded compressed tar file). Invited review at IAU Colloquium 158 "Cataclysmic Variables and Related Objects", Keele. 26-30 June 1995
Cited by in corpus (7)
- The disc instability model for X-ray transients: evidence for truncation and irradiation
- Advection-Dominated Flows and the X-ray Delay in the Outburst of GRO J1655-40
- A Population of Faint Non-Transient Low Mass Black Hole Binaries
- The Accretion Disk Limit Cycle Mechanism in the Black Hole X-ray Binaries: Toward an Understanding of the Systematic Effects
- Supernova Kicks, Magnetic Braking, and Neutron-Star Binaries
- ADAFs, accretion discs and outbursts in compact binaries
- Radiation from Dwarf Nova Discs