Zobrazeno 1 - 10
of 64
pro vyhledávání: '"S. V. Zharikov"'
Autor:
A. S. Nodyarov, A. S. Miroshnichenko, S. A. Khokhlov, S. V. Zharikov, A. T. Agishev, I. A. Gabitova, N. L. Vaidman, N. Manset
Publikováno v:
The Astrophysical Journal, Vol 968, Iss 2, p 52 (2024)
HD 327083 is a binary system that consists of two supergiant components and exhibits the B[e] phenomenon. In this paper, we report the determination of a new set of the system’s fundamental parameters using a combination of photometric and spectros
Externí odkaz:
https://doaj.org/article/c141376cb64c43c3b9a440157243043b
Autor:
A. K. Kuratova, A. S. Miroshnichenko, S. V. Zharikov, N. Manset, S. A. Khokhlov, A. Raj, A. V. Kusakin, I. V. Reva, R. I. Kokumbaeva, I. A. Usenko, A. Y. Knyazev
Publikováno v:
Odessa Astronomical Publications, Vol 32, Iss 0, Pp 63-65 (2019)
Objects with the B[e] phenomenon exhibit permitted and forbidden emission lines due to the presence of circumstellar ionized gas and large infrared excesses due to processing of the stellar radiation by circumstellar dust. There are five groups of st
Externí odkaz:
https://doaj.org/article/508c93b96b514323b4e921e55e178c85
Autor:
A. S. Miroshnichenko, N. Manset, S. V. Zharikov, J. Zsargó, J. A. Juárez Jiménez, J. H. Groh, H. Levato, M. Grosso, R. J. Rudy, E. A. Laag, K. B. Crawford, R. C. Puetter, D. E. Reichart, K. M. Ivarsen, J. B. Haislip, M. C. Nysewander, A. P. LaCluyze
Publikováno v:
Advances in Astronomy, Vol 2014 (2014)
We present spectroscopic and photometric observations of the emission-line star MWC 930 (V446 Sct) during its long-term optical brightening in 2006–2013. Based on our earlier data we suggested that the object has features found in Luminous Blue Var
Externí odkaz:
https://doaj.org/article/7fbc83f7bf3d4b6aa357e7df6d849134
Autor:
S A. Khokhlov, A. S. Miroshnichenko, S. V, Zharikov, N. Manset, O. V. Zakhozhay, I. O. Bilinskyi, K. N. Grankin, A. V. kusakin, C. T. Omarov, R. I, Kokumbaeva, I. V. Reva, D. Korcakova, I. A. Usenko, A. K. Kuratova
Publikováno v:
Odessa Astronomical Publications, Vol 33, Iss 0, Pp 141-146 (2020)
The all-sky survey conducted by the InfraRed Astronomical Satellite (IRAS) in the 1980’s discovered many objects with infrared excesses whose nature has not been explored until recently. IRAS07080+0605 is one of those identified in the visual spect
Externí odkaz:
https://doaj.org/article/70fd3e9f02ee4b148080a5941ddd2989
Autor:
E. A. Barsukova, A. N. Burenkov, V. P. Goranskij, S. V. Zharikov, L. Iliev, N. Manset, N. V. Metlova, A. S. Miroshnichenko, A. V. Moiseeva, P. L. Nedialkov, E. A. Semenko, K. Stoyanov, I. A. Yakunin
Publikováno v:
Astrophysical Bulletin. 78:1-24
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1e11a5cfd2c3c01e6232816e8c934276
https://doi.org/10.1134/s1990341323010029
https://doi.org/10.1134/s1990341323010029
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:
M. S. Hernandez, D. Steeghs, Pablo Rodríguez-Gil, S. V. Zharikov, A. Aungwerojwit, G. H. Tovmassian, Boris T. Gänsicke
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 503:1431-1441
We analysed a wealth of optical spectroscopic and photometric observations of the bright (V=11.9) cataclysmic variable BG Tri. TheGaiaDR2 parallax gives a distance d=334(8)pc to the source, making the object one of the intrinsically brightest nova-li
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::170fbaff3c45f77a6377ca24cd90b8da
https://doi.org/10.1093/mnras/stab301
https://doi.org/10.1093/mnras/stab301
Autor:
I. V. Reva, Ch. T. Omarov, I. O. Bilinskyi, A. S. Miroshnichenko, Nadine Manset, I. A. Usenko, O. V. Zakhozhay, K. N. Grankin, S. A. Khokhlov, A. V. Kusakin, D. Korcakova, R. I. Kokumbaeva, S. V. Zharikov, A. K. Kuratova
Publikováno v:
Odessa Astronomical Publications, Vol 33, Iss 0, Pp 141-146 (2020)
Odessa Astronomical Publications; Том 33 (2020); 141-146
Odessa Astronomical Publications; Том 33 (2020); 141-146
The all-sky survey conducted by the InfraRed Astronomical Satellite (IRAS) in the 1980’s discovered many objects with infrared excesses whose nature has not been explored until recently. IRAS07080+0605 is one of those identified in the visual spect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6de8705f380cecc6ca1fa1965cfe7a4a
https://doi.org/10.18524/1810-4215.2020.33.216403
https://doi.org/10.18524/1810-4215.2020.33.216403
Autor:
S. V. Zharikov, M. S. Hernandez, G. H. Tovmassian, S. A. Khokhlov, G. Subebekova, Hana Kučáková, Marek Wolf, Vitaly Neustroev
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 497:1475-1487
We obtained photometric observations of the nova-like cataclysmic variable RW Tri and gathered all available AAVSO and other data from the literature. We determined the system parameters and found their uncertainties using the code developed by us to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7ce49245b62137bf2838895b6756c93f
https://doi.org/10.1093/mnras/staa2091
https://doi.org/10.1093/mnras/staa2091
Autor:
A. S. Nodyarov, A. S. Miroshnichenko, S. A. Khokhlov, S. V. Zharikov, N. Manset, V. G. Klochkova, K. N. Grankin, A. A. Arkharov, N. Efimova, S. Klimanov, V. M. Larionov, R. J. Rudy, R. C. Puetter, R. B. Perry, I. V. Reva, C. T. Omarov, R. I. Kokumbaeva
Publikováno v:
The Astrophysical Journal. 936:129
We present the results of optical and near-IR spectroscopy and multicolor photometry of the emission-line star MWC 645, which exhibits the B[e] phenomenon. The presence of positionally variable absorption lines of a cool star detected for the first t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8f5f88cd2617164e01ee19325c2336d5
https://doi.org/10.3847/1538-4357/ac87a1
https://doi.org/10.3847/1538-4357/ac87a1