Zobrazeno 1 - 10
of 30
pro vyhledávání: '"G. V. Lipunova"'
Autor:
V. M. Lipunov, V. A. Sadovnichy, M. I. Panasyuk, I. V. Yashin, S. I. Svertilov, S. G. Simakov, D. Svinkin, E. Gorbovskoy, G. V. Lipunova, V. G. Kornilov, D. Frederiks, V. Topolev, R. Rebolo, M. Serra, N. Tiurina, E. Minkina, V. V. Bogomolov, A. V. Bogomolov, A. F. Iyudin, A. Chasovnikov, A. Gabovich, A. Tsvetkova, N. M. Budnev, O. A. Gress, G. Antipov, I. Gorbunov, D. Vlasenko, P. Balanutsa, R. Podesta, K. Zhirkov, A. Kuznetsov, V. Vladimirov, F. Podesta, C. Francile, Yu. Sergienko, A. Tlatov, O. Ershova, D. Cheryasov, V. Yurkov, A. V. Krylov
Publikováno v:
The Astrophysical Journal, Vol 943, Iss 2, p 181 (2023)
This article presents the early results of synchronous multiwavelength observations of one of the brightest gamma-ray bursts (GRBs) GRB 160625B with the detailed continuous fast optical photometry of its optical counterpart obtained by MASTER and wit
Externí odkaz:
https://doaj.org/article/4e9448e162ee4edfb2c7c46caf04d854
Autor:
G. V. Lipunova, N. I. Shakura
Publikováno v:
Odessa Astronomical Publications, Vol 12, Iss 0, Pp 201-204 (2017)
The analytic investigation of time dependent accretion in disk is carried out. We consider a disk in a binary system at outburst which has fixed tidally truncated outer radius. The standard model (Shakura-Sunyaev 1973) of the disk is considered. The
Externí odkaz:
https://doaj.org/article/3d8451e53afe4e31985cec9799ec144d
Multiwavelength observations of GRB160625B by MASTER, Lomonosov, Konus-Wind and three stage collapse
Autor:
V. M. Lipunov, V. A. Sadovnichy, M. I. Panasyuk, I. V. Yashin, S. I. Svertilov, D. Svinkin, E. Gorbovskoy, S. G. Simakov, G. V. Lipunova, V. G. Kornilov, D. Frederiks, V. Topolev, R. Rebolo, M. Serra, N. Tiurina, E. Minkina, V. V. Bogomolov, A. V. Bogomolov, A. F. Iyudin, A. Chasovnikov, A. Gabovich, N.M. Budnev, O. A. Gress, G. Antipov, D. Vlasenko, P. Balanutsa, R. Podesta, K. Zhirkov, A. Kuznetsov, V. Vladimirov, F. Podesta, C. Francile, Yu. Sergienko, A. Tlatov, O. Ershova, D. Cheryasov, V. Yurkov
Publikováno v:
The Sixteenth Marcel Grossmann Meeting.
Publikováno v:
Astronomy Letters. 47:377-389
We consider a new mechanism for the removal of the angular momentum from an X-ray binary system and the change in its orbital period - the mass loss in the form of a wind from an accretion disc. Both observations and models predict powerful winds fro
Autor:
M. I. Gornostaev, G. V. Lipunova
The problem under consideration is to determine the change of the cosmic microwave background (CMB) spectral shape due to the thermal Sunyaev–Zeldovich (tSZ) effect. We numerically model the spectral intensity of the CMB radiation Comptonized by th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::62c1b535885dc9719c287acccdafc411
http://arxiv.org/abs/2009.14698
http://arxiv.org/abs/2009.14698
Autor:
E. S. Gorbovskoy, G. V. Lipunova, V. G. Kornilov, D. Vlasenko, V. M. Lipunov, N. V. Tyurina, Ivan Panchenko, V. Grinshpun
Publikováno v:
New Astronomy. 63:48-60
The Multimessenger GW170817 / GRB170817A discovery of the merger of two neutron stars on 17th August 2017 accompanied by a gamma-ray burst and an optical kilonova event is a triumph of the ideas about the evolution of the baryon component in the Univ
Autor:
G. V. Lipunova, Adam Ingram, Alexander A. Mushtukov, Sergey S. Tsygankov, Juhani Mönkkönen, Michiel van der Klis
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 486(3), 4061-4074. Oxford University Press
Monthly Notices of the RAS (0035-8711), 486(3), 4061-4074
Monthly Notices of the RAS (0035-8711), 486(3), 4061-4074
We investigate aperiodic X-ray flux variability in accreting highly magnetized neutron stars - X-ray pulsars (XRPs). The X-ray variability is largely determined by mass accretion rate fluctuations at the NS surface, which replicate accretion rate flu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c25f0948b167c99c355fa5445964067b
http://arxiv.org/abs/1904.01132
http://arxiv.org/abs/1904.01132
We present a model for a super-Eddington accretion disc around a magnetized neutron star taking into account advection of heat and the mass loss by the wind. The model is semi-analytical and predicts radial profiles of all basic physical characterist
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fd7f38bc3c25bab7c24517975b1ff86b
Publikováno v:
The multi-messenger astronomy: gamma-ray bursts, search for electromagnetic counterparts to neutrino events and gravitational waves. Proceedings of the International Conference..
Publikováno v:
The multi-messenger astronomy: gamma-ray bursts, search for electromagnetic counterparts to neutrino events and gravitational waves. Proceedings of the International Conference..