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DIM light on Black Hole X-ray Transients

Abstract : The current model for the outburst of stellar-mass black holes X-ray binaries is the disk instability model (DIM). An overview of this model and a discussion of its theoretical and observational challenges are given.
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Contributor : Dominique Girod <>
Submitted on : Tuesday, October 31, 2006 - 9:21:07 AM
Last modification on : Thursday, March 5, 2020 - 6:19:27 PM

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G. Dubus. DIM light on Black Hole X-ray Transients. Astrophysical Sources of High Energy Particles and Radiation, Jun 2005, Torun, Poland. pp.153-158, ⟨10.1063/1.2141853⟩. ⟨in2p3-00110592⟩



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