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Models of Soft X-Ray Transients and Dwarf Novae
1996
International Astronomical Union Colloquium
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AbstractModels 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.
doi:10.1017/s0252921100039221
fatcat:lfpvevgah5c6loyxfrylwqo3fa