Výsledky vyhledávání - "PUSTIL'NIK L. A"

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A new look at the origin of the 6.67\,hr period X-ray pulsar 1E~161348-5055

Autor: Ikhsanov, N. R., Kim, V. Y., Beskrovnaya, N. G., Pustil'nik, L. A.

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 RCW\,103 and is widely believed to be a ~2000 yr old neutron star. Obser

Externí odkaz: http://arxiv.org/abs/1212.0375

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Magnetically controlled accretion onto a black hole

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

Publikováno v: Journal of Physics: Conference Series, Volume 372, Issue 1, pp. 012062 (2012)

An accretion scenario in which the material captured by a black hole from its environment is assumed to be magnetized (\beta ~ 1) is discussed. We show that the accretion picture in this case is strongly affected by the magnetic field of the flow its

Externí odkaz: http://arxiv.org/abs/1211.4400

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

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

Publikováno v: AIP Conference Proceedings 1439, 237-248 (2012)

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 stellar field and spin evolution of long-period X-ray pulsars. These difficu

Externí odkaz: http://arxiv.org/abs/1205.1220

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On the energy release in solar flares

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

Publikováno v: AIP Conf. Proc. 1439, 63 (2012)

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 traditional 'potential + force-free' field scenarios. The interacting

Externí odkaz: http://arxiv.org/abs/1204.6594

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