activity
20012024
most citedDark energy and key physical parameters of clusters of galaxies

16 citations · 35 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2024★ 10 cited

Magnetorotational neutron star kicks

Ilya A. Kondratyev, Sergey G. Moiseenko, Gennady S. Bisnovatyi-Kogan

High velocity neutron stars, observed as rapidly moving radio-pulsars, are believed to gain high linear velocities -- kicks -- in aspherical supernova explosions. The mechanism of…

astro-ph.HE2014

Optical and X-ray behaviour of the high mass X-ray transient A0535+26/HDE245770 in February-March 2014

F. Giovannelli, G. S. Bisnovatyi-Kogan, I. Bruni +3

The optical behaviour of the Be star in the high-mass X-ray transient A0535+26/HDE245770 shows that at periastron the luminosity is typically enhanced by 0.02 to a few tenths magni…

astro-ph.CO2013★ 7 cited

Galactic cluster winds in presence of a dark energy

G. S. Bisnovatyi-Kogan, M. Merafina

We obtain a solution for the hydrodynamic outflow of the polytropic gas from the gravitating center, in presence of the uniform Dark Energy (DE). The antigravity of DE is enlighten…

astro-ph.CO2012★ 16 cited

Dark energy and key physical parameters of clusters of galaxies

G. S. Bisnovatyi-Kogan, A. D. Chernin

We study physics of clusters of galaxies embedded in the cosmic dark energy background. Under the assumption that dark energy is described by the cosmological constant, we show tha…

astro-ph.CO2011★ 1 cited

Polytropic configurations with non-zero cosmological constant

M. Merafina, G. S. Bisnovatyi-Kogan, S. O. Tarasov

We solve the equation of the equilibrium of the gravitating body, with a polytropic equation of state of the matter , with , in the frame of the Newtonian gravity,…

astro-ph2003

Magnetorotational mechanism of supernova type II exlosion

S. G. Moiseenko, G. S. Bisnovatyi-Kogan, N. V. Ardeljan

Results of 2D simulations of the magnetorotational mechanism of supernova type II are presented. Amplification of toroidal magnetic field of the star due to differential rotation o…