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20012025
most citedNew Torque Reversal and Spin-Up of 4u 1626- 67 Observed by Fermi/GBM and Swift/BAT

61 citations · 665 across the 47 of their papers we have counts for

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21 papers · 1 filter

astro-ph.HE2017★ 2 cited

Long-term study of the Double Pulsar J0737-3039 with XMM-Newton: spectral analysis

Elise Egron, Alberto Pellizzoni, Andy Pollock +4

We present a long-term spectral monitoring of the unique Double Pulsar binary PSR J0737-3039 corresponding to two "Large Programs" performed by XMM-Newton in 2006 and 2011. Spectra…

astro-ph.HE2016★ 2 cited

AR Scorpii is a new white dwarf in the ejector state

N. G. Beskrovnaya, N. R. Ikhsanov

Marsh et al. (2016) have recently reported the discovery of a radio-pulsing white dwarf in the cataclysmic variable AR Sco. The period of pulsations which are also seen in the opti…

astro-ph.HE2014★ 5 cited

A scenario of the formation of isolated X-ray pulsars with anomalously long period

N. R. Ikhsanov, V. Yu. Kim, N. G. Beskrovnaya

A scenario of the formation of isolated X-ray pulsars is discussed with an application to one of the best studied objects of this class 1E 161348-5055. This moderately luminous, 10…

astro-ph.HE2014★ 1 cited

Period clustering of the anomalous X-ray pulsars

G. S. Bisnovatyi-Kogan, N. R. Ikhsanov

In this paper we address the question of why the observed periods of the Anomalous X-ray Pulsars (AXPs) and Soft Gamma-ray Repeaters (SGRs) are clustered in the range 2-12 s. We ex…

astro-ph.HE2014★ 2 cited

On the origin of the peculiar cataclysmic variable AE Aquarii

N. G. Beskrovnaya, N. R. Ikhsanov

The nova-like variable AE Aquarii is a close binary system containing a red dwarf and a magnetized white dwarf rotating with the period of 33 seconds. A short spin period of the wh…

astro-ph.HE2014★ 13 cited

Spin evolution of long-period X-ray pulsars

N. R. Ikhsanov, Yu. S. Likh, N. G. Beskrovnaya

Spin evolution of X-ray pulsars in High Mass X-ray Binaries (HMXBs) is discussed under various assumptions about the geometry and physical parameters of the accretion flow. The tor…