The analytic investigation of time dependent accretion in disk is carried out. We consider a disk in a binary system at outburst which has fixed tidally truncated outer radius. The standard model (Shakura-Sunyaev 1973) of the disk is considered. The fully analytic solutions in two different opacity regimes are characterized by power-law variations of accretion rate with time. The solutions supply asymptotic description of the disk evolution after the peak of outburst while the disk is fully ionized. The X-ray flux of multicolor (black-body) α-disk is obtained to vary quasi-exponentially. The application to X-ray novae is briefly discussed concerning observed faster-than-power decays of X-ray light curves. The case of time dependent advectiv...
International audienceThe X-ray light curves of the recurring outbursts observed in low-mass X-ray b...
Aims. We study the inner disk structure of dwarf novae (DNe; i.e., nonmagnetic cataclysmic variables...
The outbursts of low-mass X-ray binaries are prolonged relative to those of dwarf nova cataclysmic v...
Several black hole X-ray transients have a very long recurrence time, decades of years. We study the...
We present a method of modeling X-ray and optical light curves of time-dependent accretion α-disks i...
We propose a new model for X-ray spectral fitting of binary black hole candidates. In this model, it...
We have fit outbursts of two X-ray novae (Nova Monocerotis 1975 = A 0620-00 and Nova Muscae GS 1991 ...
Based on previous works on black hole accretion disks, I continue to explore the disk dynamics using...
The outburst cycles of black hole X-ray transients are now generally understood as caused by a therm...
We examine in detail several aspects of the physics of accretion disks of possible relevance to the ...
I review recent advances in our understanding of accretion disks in transient systems - the dwarf no...
The outburst cycles of black hole X-ray transients are now generally understood as caused by a therm...
In a supermassive black hole (BH) tidal disruption event (TDE), the tidally disrupted star feeds the...
Abstract: We consider a new mechanism for the removal of angular momentum from an X-ray binary syste...
Aims. We address the task of modeling soft X-ray and optical light curves of X-ray novae in the high...
International audienceThe X-ray light curves of the recurring outbursts observed in low-mass X-ray b...
Aims. We study the inner disk structure of dwarf novae (DNe; i.e., nonmagnetic cataclysmic variables...
The outbursts of low-mass X-ray binaries are prolonged relative to those of dwarf nova cataclysmic v...
Several black hole X-ray transients have a very long recurrence time, decades of years. We study the...
We present a method of modeling X-ray and optical light curves of time-dependent accretion α-disks i...
We propose a new model for X-ray spectral fitting of binary black hole candidates. In this model, it...
We have fit outbursts of two X-ray novae (Nova Monocerotis 1975 = A 0620-00 and Nova Muscae GS 1991 ...
Based on previous works on black hole accretion disks, I continue to explore the disk dynamics using...
The outburst cycles of black hole X-ray transients are now generally understood as caused by a therm...
We examine in detail several aspects of the physics of accretion disks of possible relevance to the ...
I review recent advances in our understanding of accretion disks in transient systems - the dwarf no...
The outburst cycles of black hole X-ray transients are now generally understood as caused by a therm...
In a supermassive black hole (BH) tidal disruption event (TDE), the tidally disrupted star feeds the...
Abstract: We consider a new mechanism for the removal of angular momentum from an X-ray binary syste...
Aims. We address the task of modeling soft X-ray and optical light curves of X-ray novae in the high...
International audienceThe X-ray light curves of the recurring outbursts observed in low-mass X-ray b...
Aims. We study the inner disk structure of dwarf novae (DNe; i.e., nonmagnetic cataclysmic variables...
The outbursts of low-mass X-ray binaries are prolonged relative to those of dwarf nova cataclysmic v...