Add to ORKGThe 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
We report on a consistent and comprehensive spectral analysis of the X-ray emission of 25 black hole...
International audienceThe disk instability picture gives a plausible explanation for the behavior of...
We consider transient behavior in low-mass X-ray binaries (LMXBs). We show that if this results from...
6 pages, 7 figures, sollicited talk for "Astrophysical Sources of High Energy Particles and Radiatio...
International audienceWe revisit a core prediction of the disc instability model (DIM) applied to X-...
Abstract. We suggest a new scenario to explain the outburst light curves of black hole soft X-ray tr...
We suggest a new scenario to explain the outburst light curves of black hole soft X-ray transients t...
The outburst cycles of black hole X-ray transients are now generally understood as caused by a therm...
We present a unified semi-quantitative model for the disc-jet coupling in black hole X-ray binary sy...
International audienceThis is an introduction to models of accretion discs around black holes. After...
International audienceContext. The disc instability model (DIM) successfully explains why many accre...
Soft X-ray transients that are black-hole candidates (BHCs) exhibit hysteretic spectral transitions ...
The outburst cycles of black hole X-ray transients are now generally understood as caused by a therm...
Black hole X-ray binaries are transient probably because their discs are subject to the same thermal...
Several black hole X-ray transients have a very long recurrence time, decades of years. We study the...
We report on a consistent and comprehensive spectral analysis of the X-ray emission of 25 black hole...
International audienceThe disk instability picture gives a plausible explanation for the behavior of...
We consider transient behavior in low-mass X-ray binaries (LMXBs). We show that if this results from...
6 pages, 7 figures, sollicited talk for "Astrophysical Sources of High Energy Particles and Radiatio...
International audienceWe revisit a core prediction of the disc instability model (DIM) applied to X-...
Abstract. We suggest a new scenario to explain the outburst light curves of black hole soft X-ray tr...
We suggest a new scenario to explain the outburst light curves of black hole soft X-ray transients t...
The outburst cycles of black hole X-ray transients are now generally understood as caused by a therm...
We present a unified semi-quantitative model for the disc-jet coupling in black hole X-ray binary sy...
International audienceThis is an introduction to models of accretion discs around black holes. After...
International audienceContext. The disc instability model (DIM) successfully explains why many accre...
Soft X-ray transients that are black-hole candidates (BHCs) exhibit hysteretic spectral transitions ...
The outburst cycles of black hole X-ray transients are now generally understood as caused by a therm...
Black hole X-ray binaries are transient probably because their discs are subject to the same thermal...
Several black hole X-ray transients have a very long recurrence time, decades of years. We study the...
We report on a consistent and comprehensive spectral analysis of the X-ray emission of 25 black hole...
International audienceThe disk instability picture gives a plausible explanation for the behavior of...
We consider transient behavior in low-mass X-ray binaries (LMXBs). We show that if this results from...