Zobrazeno 1 - 10
of 123
pro vyhledávání: '"Bogdanov, M. B."'
Autor:
Bogdanov, M. B., Cherepashchuk, A. M.
Publikováno v:
Astrophys.Space Sci.317:181-192,2008
We consider small-scale spheroidal clusters of weakly interacting massive particles in our Galaxy as non-compact gravitational microlenses and predict the appearance of caustics in the plane of a lensed source. The crossing of these caustics by a len
Externí odkaz:
http://arxiv.org/abs/0807.2774
Autor:
Bogdanov, M. B., Cherepashchuk, A. M.
We carried out numerical experiments on the evaluation of the possibilities of obtaining the information about brightness distributions for the components of eclipsing variables from the data of high-precision photometry expected for planned satellit
Externí odkaz:
http://arxiv.org/abs/astro-ph/0607250
Autor:
Bogdanov, M. B.
For an analysis of microlensing observational data in case of binary gravitational lenses as well as for an interpretation of observations of high magnification events in multiple images of a lensed quasar it is necessary to calculate for a given sou
Externí odkaz:
http://arxiv.org/abs/astro-ph/0102031
Autor:
Bogdanov, M. B.
The problem of restoration of the source brightness distribution from an analysis of the stellar and AGNs microlensing light curves is investigated. In case of microlensing of stars by a point-mass lens as well as for caustic crossing events for bina
Externí odkaz:
http://arxiv.org/abs/astro-ph/0009228
Akademický článek
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Publikováno v:
Astronomy Reports. Jul2010, Vol. 54 Issue 7, p620-627. 8p. 4 Charts, 4 Graphs.
Autor:
Bogdanov, M. B.1 BogdanovMB@info.sgu.ru, Cherepashchuk, A. M.2
Publikováno v:
Astrophysics. Oct2008, Vol. 51 Issue 4, p506-516. 11p. 1 Chart, 6 Graphs.
Autor:
Bogdanov, M. B.1, Taranova, O. G.2
Publikováno v:
Astronomy Reports. May2008, Vol. 52 Issue 5, p403-408. 6p. 2 Charts, 3 Graphs.
Autor:
Bogdanov, M. B.1 BogdanovMB@info.sgu.ru, Cherepashchuk, A. M.2
Publikováno v:
Astronomical & Astrophysical Transactions. 2007, Vol. 26 Issue 1-3, p151-158. 8p. 2 Charts, 6 Graphs.