publication . Conference object . Preprint . 2005

DIM light on Black Hole X‐ray Transients

Dubus, G.;
Open Access
  • Published: 20 Jun 2005 Journal: AIP Conference Proceedings (issn: 0094-243X, Copyright policy)
  • Publisher: AIP
  • Country: France
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.
Subjects
arXiv: Astrophysics::High Energy Astrophysical PhenomenaAstrophysics::Solar and Stellar AstrophysicsGeneral Relativity and Quantum CosmologyAstrophysics::Galaxy AstrophysicsAstrophysics::Earth and Planetary Astrophysics
free text keywords: Physics, Astrophysics, Stellar black hole, Intermediate-mass black hole, X-ray binary, Astronomy, Instability, X-ray, Black hole, X-ray binaries, Infall, accretion, and accretion disks, 97.80.Jp, 98.62.Mw, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
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