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N. G. Beskrovnaya

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • last author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
  • astro-ph.SR1
ORCID 0000-0003-4454-6729

identity via Semantic Scholar / OpenAlex

most citedAE Aquarii represents a new subclass of Cataclysmic Variables

17 citations · 36 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2012★ 17 cited

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…

astro-ph.HE2012★ 17 cited

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…

astro-ph.HE2012★ 2 cited

A new look at spherical accretion in High Mass X-ray Binaries

N. R. Ikhsanov, L. A. Pustil'nik, N. G. Beskrovnaya

Currently used model of spherical accretion onto a magnetized rotating neutron star encounters major difficulties in explaining the entry rate of accreting material into the stella…

astro-ph.SR2012

On the energy release in solar flares

L. A. Pustil'nik, N. R. Ikhsanov, N. G. Beskrovnaya

High-resolution observations show the fine structure of the global equilibrium magnetic field configuration in solar atmosphere to be essentially different from that assumed in the…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.