Zobrazeno 1 - 10
of 46
pro vyhledávání: '"V. F. Suleimanov"'
Autor:
I. L Andronov, K. Arai, L. L. Chinarova, N. I. Dorokhov, T. N. Dorokhova, A. Dumitrescu, D. Nogami, S. V. Kolesnikov, A. Lepardo, P. A. Mason, K. Matsumoto, G. Oprescu, G. Pajdosz, R. Passuelo, L. Patkos, D. S. Senio, G. Sostero, V. F. Suleimanov, J. Tremko, G. V. Zhukov, S. Zola
Publikováno v:
Odessa Astronomical Publications, Vol 10, Iss 0, Pp 10-14 (2017)
Results obtained during the international observational campaign ” Т Т Ari-94” are briefly discussed. During 258 hours, totally 51299 observations were obtained in 12 observatories. The moments of 68 individual maxima and 74 minima are tabulate
Externí odkaz:
https://doaj.org/article/823ef66593684429847a6acbe9b3fd73
Autor:
V. F. Suleimanov, I. F. Bikrnaev, C. V. Belyakov, N. A. Sakhibullin, G. V. Zhukov, Z. Aslan, U. Kizilogly, I. Kharnitov
Publikováno v:
Odessa Astronomical Publications, Vol 16, Iss 0, Pp 81-84 (2017)
The rezults of the novalike variable V603 Aql photometric observations performed by Russian-Turkish telescope RTT150 during 11 nights of 2001 - 2002 are presented. It is shown the star was in the state with ”positive” superhumps and photometric p
Externí odkaz:
https://doaj.org/article/0ccc7a0462184a3d9143be70d222b2f9
Publikováno v:
Acta Polytechnica CTU Proceedings, Vol 2, Iss 1, Pp 143-147 (2015)
The X-ray spectrum of SS Cyg in outburst has a very soft component that can be interpreted as the fast-rotating optically thick boundary layer on the white dwarf surface. This component was carefully investigated by Mauche (2004) using the Chandra LE
Externí odkaz:
https://doaj.org/article/7ca4938385564110930f749a4711b34d
Publikováno v:
Odessa Astronomical Publications, Vol 9, Iss 0, Pp 57-58 (2017)
Simultaneous WBVR photometric observations of TT Ari during 94 / 95 years are presented. The periodogram analysis of the obtained light curves and colours are curried out. The photometric period equal 3.2 h and its one day aliases are found from ligh
Externí odkaz:
https://doaj.org/article/b3aeafd6920d41ec80a666e8da9e28ab
Autor:
V. F. Suleimanov, V. V. Shimansky
Publikováno v:
Odessa Astronomical Publications, Vol 9, Iss 0, Pp 55-56 (2017)
Results of X-ray Novae (XN) optical spectra computation are presented. The continuum and Balmer line are calculated. The model of XN as a self-irradiated accretion disk is used. Local (for given radius) disk atmospheres as model stellar atmospheres,
Externí odkaz:
https://doaj.org/article/5614dcb8d51f4e9aa59ba9526f97e01a
Autor:
D A Zyuzin, S V Zharikov, A V Karpova, A Yu Kirichenko, Yu A Shibanov, S Geier, A Y Potekhin, V F Suleimanov, A Cabrera-Lavers
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 513:6088-6094
The 840 kyr old pulsar PSR J1957+5033, detected so far only in $\gamma$- and X-rays, is a nearby and rather cool neutron star with a temperature of 0.2--0.3 MK, a distance of $\la$1 kpc, and a small colour reddening excess $E(B-V) \approx 0.03$. Thes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::39bbb78982cb240f996bb6d1dee3e493
https://doi.org/10.1093/mnras/stac1293
https://doi.org/10.1093/mnras/stac1293
Autor:
A. A. Mushtukov, I. D. Markozov, V. F. Suleimanov, D. I. Nagirner, A. D. Kaminker, A. Y. Potekhin, S. Portegies Zwart
Publikováno v:
Physical Review D, 105(10):103027
Compton scattering is a key process shaping spectra formation and accretion flow dynamics in accreting strongly magnetized neutron stars. A strong magnetic field affects the scattering cross section and makes it dependent on photon energy, momentum,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::76081692d40b85850facaf4a024cc641
Autor:
V. Rana, D. J. K. Buisson, Aarran W. Shaw, John A. Tomsick, Craig O. Heinke, Renee M. Ludlam, V. F. Suleimanov, G. R. Sivakoff, Jeremy Hare, Koji Mukai, Poshak Gandhi, Victor Doroshenko, Brian W. Grefenstette, Jiachen Jiang
The hard X-ray spectrum of magnetic cataclysmic variables can be modelled to provide a measurement of white dwarf mass. This method is complementary to radial velocity measurements, which depend on the (typically rather uncertain) binary inclination.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::551909e8e909337830d15fb951664cae
https://resolver.caltech.edu/CaltechAUTHORS:20201209-153311091
https://resolver.caltech.edu/CaltechAUTHORS:20201209-153311091
Autor:
G. H. Gao, X. X. Li, M. Wu, S. J. Zheng, Y. G. Zheng, Y. Nang, Mauro Orlandini, J. Y. Liao, H. M. Zhang, Y. L. Tuo, Y. J. Yang, R. C. Ma, Y. F. Zhang, X. B. Li, B. S. Liu, Yuan You, X. Q. Ren, Yanji Yang, Armin Nabizadeh, C. Cai, L. Chen, Tian-Xiang Chen, Wenxiong Li, Wan-Chang Zhang, W. S. Wang, Yi Zhang, Ge Ou, Andrea Santangelo, R. J. Yang, Bo Li, Peng Zhang, Qiu-Yi Luo, B. B. Wu, Cunguo Wang, H. S. Zhao, Li-Ming Song, Ming-Yu Ge, C. K. Li, F. J. Lu, Xue-Feng Lu, Y. P. Chen, Shuinai Zhang, Tong Li, Y. H. Tan, P. J. Wang, J. Y. Zhang, Victor Doroshenko, Shaolin Xiong, S. M. Jia, XiangYang Wen, Ling-Jun Wang, H. Gao, Jiren Liu, X. H. Ma, Z. W. Li, Yuan-Yuan Du, C. Z. Liu, D. K. Zhou, Sisi Yang, Ya Fang Huang, J. Jin, Xin-Fu Zhao, G. Li, Tao Luo, S. Xiao, Yu-Dong Gu, X. J. Liu, D. Gavran, X. L. Cao, Q. Q. Yin, Q. B. Yi, B. Y. Wu, V. F. Suleimanov, L. D. Kong, Y. B. Chen, X. H. Liang, L. Sun, Fuqin Zhang, S. N. Zhang, Long Ji, Z. Chang, Y. H. Zhang, Y. P. Xu, Wenhan Jiang, H. W. Liu, N. Sai, Y. S. Wang, W. C. Zhang, Xuelong Li, J. Guan, Lian Tao, Cheng-Cheng Guo, X. Y. Song, Jia Huo, Lorenzo Ducci, J. Y. Nie, Bin Meng, Wei Cui, G. C. Xiao, Qingcui Bu, Da-Wei Han, J. L. Qu, Hongfei Liu
We investigate the absorption and emission features in observations of GX 301-2 detected with Insight-HXMT/LE in 2017-2019. At different orbital phases, we found prominent Fe Kalpha, Kbeta and Ni Kalpha lines, as well as Compton shoulders and Fe K-sh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::813b3337eb5985bf4c58b738f8290cc0
Type I X-ray bursts in GS 1826–24, and in several other systems, may induce cooling of the hot inner accretion flow that surrounds the bursting neutron star. Given that GS 1826–24 remained persistently in the hard state over the period 2003–200
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a382019964be91e20dc532d09d8a41b0