167 citations · 1k across the 54 of their papers we have counts for
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Magnetic fields of isolated neutron stars: evidence for decay
S. B. Popov, M. E. Prokhorov
We show, that different types of isolated neutron stars (INSs) show evidence in favor of magnetic field decay in these objects, and discuss how observations of INSs can help to con…
Broad-band gravitational-wave pulses from binary neutron stars in eccentric orbits
A. V. Gusev, V. B. Ignatiev, A. G. Kuranov +2
Maximum gravitational wave emission from binary stars in eccentric orbits occurs near the periastron passage. We show that for a stationary distribution of binary neutron stars in…
Why NS and BH mass distribition is bimodal?
M. E. Prokhorov, K. A. Postnov
The observed mass distribution for the compact remnants of massive stars (neutron stars and black holes) and its relationship to possible mechanisms for the ejection of the envelop…
Stochastic spin evolution of neutron stars
S. B. Popov, M. E. Prokhorov, A. V. Khoperskov +1
In this paper we present calculations of period distribution for old accreting isolated neutron stars (INSs). At the age about a few billions years low velocity INSs come to the st…
Period distribution of old accreting isolated neutron stars
M. E. Prokhorov, S. B. Popov, A. V. Khoperskov
In this paper we present calculations of period distribution for old accreting isolated neutron stars (INSs). After few billion years of evolution low velocity INSs come to the sta…
Gravitational wave background from coalescing compact stars in eccentric orbits
V. B. Ignatiev, A. G. Kuranov, K. A. Postnov +1
Stochastic gravitational wave background produced by a stationary coalescing population of binary neutron stars in the Galaxy is calculated. This background is found to constitute…
Evolution of isolated neutron stars in globular clusters: number of Accretors
S. B. Popov, M. E. Prokhorov
With a simple model from the point of view of population synthesis we try to verify an interesting suggestion made by Pfahl & Rappaport (2001) that dim sources in globular clusters…