61 citations · 665 across the 47 of their papers we have counts for
9 papers · 1 filter
A new look at the origin of the 6.67\,hr period X-ray pulsar 1E~161348-5055
N. R. Ikhsanov, V. Y. Kim, N. G. Beskrovnaya +1
The point X-ray source 1E 161348-5055 is observed to display pulsations with the period 6.67 hr and |\dot{P}| \leq 1.6 x 10^{-9} s/s. It is associated with the supernova remnant RC…
On the spin-down mechanism of the X-ray pulsar 4U 2206+54
N. R. Ikhsanov, N. G. Beskrovnaya
Observations of the X-ray pulsar 4U 2206+54, performed over a 15-year span, show its period, which is now 5555 \pm 9 s, to increase drastically. Such behavior of the pulsar can be…
Magnetically controlled accretion onto a black hole
N. R. Ikhsanov, L. A. Pustil'nik, N. G. Beskrovnaya
An accretion scenario in which the material captured by a black hole from its environment is assumed to be magnetized (β~ 1) is discussed. We show that the accretion picture in thi…
Signs of magnetic accretion in young Be/X-ray pulsar SXP 1062
N. R. Ikhsanov
The spin behaviour of the neutron star in the newly discovered young Be/X-ray long-period pulsar SXP 1062 is discussed. The star is observed to rotate with the period of 1062s, and…
AE Aquarii represents a new subclass of Cataclysmic Variables
N. R. Ikhsanov, N. G. Beskrovnaya
We analyze properties of the unique nova-like star AE Aquarii identified with a close binary system containing a red dwarf and a very fast rotating magnetized white dwarf. It canno…
Signs of magnetic accretion in X-ray pulsars
N. R. Ikhsanov, N. G. Beskrovnaya
The spin-down mechanism of accreting neutron stars is discussed with an application to one of the best studied X-ray pulsars GX 301-2. We show that the maximum possible spin-down t…