Zobrazeno 1 - 10
of 73
pro vyhledávání: '"Abubekerov, M. K."'
Autor:
Bekesov, E. V.1 (AUTHOR), Abubekerov, M. K.1 (AUTHOR) marat@sai.msu.ru, Gostev, N. Yu.1 (AUTHOR) ngostev@mail.ru, Cherepashchuk, A. M.1 (AUTHOR) cherepashchuk@gmail.com
Publikováno v:
Astronomy Reports. Nov2023, Vol. 67 Issue 11, p1096-1122. 27p.
Autor:
Abubekerov, M. K.1 (AUTHOR) marat@sai.msu.ru, Gostev, N. Yu.1 (AUTHOR) ngostev@mail.ru
Publikováno v:
Astronomy Reports. Jun2023, Vol. 67 Issue 6, p547-553. 7p.
Autor:
Abubekerov, M. K., Gostev, N. Yu.
Publikováno v:
Astronomy Reports; Jul2024, Vol. 68 Issue 7, p641-649, 9p
Autor:
Abubekerov, M. K., Gostev, N. Yu.
We have developed a universal approach to compute accurately the brightness of eclipsing binary systems during the transit of a planet in front of the stellar disk. This approach is uniform for all values of the system parameters and applicable to mo
Externí odkaz:
http://arxiv.org/abs/1304.1378
Publikováno v:
Astronomy Reports, 2008, Vol.52, pp.379-389
We have obtained the first estimates of the masses of the components of the Her X-1/HZ Her X-ray binary system taking into account non-LTE effects in the formation of the H_gamma absorption line: mx=1.8Msun and mv=2.5Msun. These mass estimates were m
Externí odkaz:
http://arxiv.org/abs/1201.5519
Publikováno v:
Astronomy Reports, 2006, Vol.50, No.7, pp. 544--552
We interpret the observed radial-velocity curve of the optical star in the low-mass X-ray binary 2S 0921-630 using a Roche model, taking into account the X-ray heating of the optical star and screening of X-rays coming from the relativistic object by
Externí odkaz:
http://arxiv.org/abs/1201.4689
Publikováno v:
Astronomy Reports, 2011, Vol.55, pp.1051-1073
High-accuracy multicolor light curves of the binary system HD 189733, which contains an exoplanet, are analyzed. We have determined the radii of the star and the planet in the binary system, as well as the orbital inclination. The limb-darkening coef
Externí odkaz:
http://arxiv.org/abs/1201.4043
Autor:
Abubekerov, M. K.1 (AUTHOR) marat@sai.msu.ru, Gostev, N. Yu.1 (AUTHOR) ngostev@mail.ru
Publikováno v:
Astronomy Reports. Nov2022, Vol. 66 Issue 11, p919-924. 6p.
Publikováno v:
Astron.Rep.53:232-242,2009
We have analyzed the observed radial-velocity curve for the X-ray binary M33 X-7 in a Roche model. We have analyzed the dependence between the component masses and the degree of filling of the optical star's Roche lobe to obtain the ratio of the mass
Externí odkaz:
http://arxiv.org/abs/0906.3429
Publikováno v:
Mon.Not.Roy.Astron.Soc. 359 (2005) 1517-1523
Using "Scenario Machine" we have carried out population synthesis of radio pulsar with black hole binaries (BH+Psr) in context of the most wide assumptions about star mass loss during evolution, binary stars mass ratio distribution, kick velocity and
Externí odkaz:
http://arxiv.org/abs/astro-ph/0503341