48 citations · 56 across the 4 of their papers we have counts for
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AE Aquarii: The first white dwarf in the family of spin-powered pulsars
N. R. Ikhsanov, N. G. Beskrovnaya
Simulation of Doppler H-alpha tomogram of the nova-like star AE Aquarii suggests that the dipole magnetic moment of the white dwarf is close to 1.5E+34 G cm^3. This is consistent w…
Accreting isolated neutron stars
N. R. Ikhsanov, P. L. Biermann
Accretion of interstellar material by a magnetized, slowly rotating isolated neutron star is discussed. We show that the average persistent X-ray luminosity of these objects is unl…
The origin of long-period X-ray pulsars
N. R. Ikhsanov
Several relatively bright, persistent X-ray sources display regular pulses, with periods in the range of 700-10000 s. These sources are identified with massive close binaries in wh…
On a Site of X-ray Emission in AE Aquarii
N. R. Ikhsanov
An analysis of recently reported results of XMM-Newton observations of AE Aqr within a hypothesis that the detected X-ray source is located inside the Roche lobe of the white dwarf…
High-energy emission of fast rotating white dwarfs
N. R. Ikhsanov, P. L. Biermann
The process of energy release in the magnetosphere of a fast rotating, magnetized white dwarf can be explained in terms of the canonical spin-powered pulsar model. Applying this mo…
On the mass transfer in AE Aquarii
N. R. Ikhsanov, V. V. Neustroev, N. G. Beskrovnaya
The observed properties of the close binary AE Aqr indicate that the mass transfer in this system operates via the Roche lobe overflow mechanism, but the material transferred from…