Accretion heated atmospheres of X-ray bursting neutron stars that these deviations are induced by the additional heating of the
accreted particles. We present a method
Colors and patterns of black hole X-ray binary GX 339-4 temperatures of the
accretion disk. We show that various spectral states of regular outbursts occupy similar
The boundary layer in compact binariesContext. Disk
accretion onto stars leads to the formation of a boundary layer (BL) near the stellar
Vertical structure of the outer accretion disk in persistent low-mass X-ray binaries accretion disk in low-mass X-ray binaries by performing a self-consistent calculation of the vertical
Observations of GRO J1744-28 in quiescence with XMM-Newton law, blackbody, or
accretion-heated neutron star atmosphere models. The improved X-ray localization
X-ray variability of the HMXB Cen X-3: Evidence for inhomogeneous accretion flows of the
accretion stream. The second observation was taken when the source was 10 times X-ray brighter and covered
Ya.B. Zeldovich and Foundation of the Accretion Theory Zeldovich, the science of his epoch and the creation of modern
accretion theory.