activity
20052026
most citedSuper-critically accreting stellar-mass black holes as ultraluminous X-ray sources

554 citations · 1.1k across the 46 of their papers we have counts for

collaborators

47 papers

astro-ph.HE2026

Pulse profiles of tall accretion columns in X-ray pulsars

Bagration Megrelishvili, Pavel Abolmasov

Accreting X-ray pulsars (XRPs) are strongly magnetized neutron stars (NSs) distinguished by a periodic variability pattern related to the rotation of their magnetospheres (pulsatio…

astro-ph.HE2026

Variable opacity and accretion-column regimes of magnetized neutron stars

Galina Lipunova, Pavel Abolmasov

Radiation-supported accretion columns of magnetized neutron stars can operate in several distinct regimes. As the accretion rate increases, magnetospheric accretion may proceed thr…

astro-ph.HE2026

Shock-free super-Eddington accretion onto magnetized neutron star

Galina Lipunova, Pavel Abolmasov

Strong magnetic fields allow accreting neutron stars to form magnetically controlled funnel flows. At sufficiently high accretion rates, such flows become radiation-pressure-suppor…

astro-ph.HE2024

Numerical approach to compressible shallow-water dynamics of neutron-star spreading layers

Aleksandr Rusakov, Pavel Abolmasov, Omer Bromberg

A weakly magnetized neutron star (NS) undergoing disk accretion should release about a half of its power in a compact region known as the accretion boundary layer. Latitudinal spre…

astro-ph.HE2022★ 16 cited

Interface instabilities in hydrodynamic relativistic jets

Pavel Abolmasov, Omer Bromberg

Both the dynamics and the observational properties of relativistic jets are determined by their interaction with the ambient medium. A crucial role is played by the contact discont…

astro-ph.HE2022★ 16 cited

Simulating the shock dynamics of a neutron star accretion column

Pavel Abolmasov, Galina Lipunova

Accretion onto a highly-magnetised neutron star runs through a magnetospheric flow, where the plasma follows the magnetic field lines in the force-free regime. The flow entering th…