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First simultanous X-ray and optical observations of rapid variability of supercritical accretor SS433 of mass accretion rate perturbations from the jet base to the observed X-ray emitting region

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

Non-LTE models for neutron star atmospheres and supernova-fallback disksAccretion

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.

Accreting millisecond pulsar SAX J1808.4-3658 during its 2002 outburst: Evidence for a receding discAn outburst of the accreting X-ray millisecond pulsar SAX J1808.4-3658 in 2002 October

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