Zobrazeno 1 - 10
of 61
pro vyhledávání: '"Chulkov, D."'
Autor:
Malkov, O. Yu., Kovaleva, D. A., Yungelson, L. R., Avvakumova, E. A., Chulkov, D. A., Dluzhnevskaya, O. B., Kniazev, A. Yu
Publikováno v:
Baltic astronomy (2016), Vol. 25, pp. 384-392
We present results of Monte Carlo simulation aiming at the estimate of the frequency of semi-detached Algol-type binaries among the stars observed as single ones. When account is made for various detection biases (mostly due to inclination of orbits)
Externí odkaz:
http://arxiv.org/abs/1701.00746
Publikováno v:
Baltic astronomy (2016), Vol. 25, pp. 419-426
Statistics of orbital parameters of binary stars as well as statistics of their physical characteristics bear traces of star formation history. However, statistical investigations of binaries are complicated by lacking or incomplete observational dat
Externí odkaz:
http://arxiv.org/abs/1701.00421
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 459, Issue 2, p.1580-1585, 2016
Improved orbits are presented for the visual binaries WDS 02366+1227, WDS 02434-6643, WDS 03244-1539, WDS 08507+1800, WDS 09128-6055, WDS 11532-1540, WDS 17375+2419, and WDS 22408-0333. The latest orbits for these binaries were demonstrating a great
Externí odkaz:
http://arxiv.org/abs/1609.03392
Publikováno v:
Astrophysics and Space Science, Volume 361, article id.105, 2016
We have selected a set of 17 visual binaries that demonstrate great inconsistency between the systemic mass obtained through Kepler's Third Law as compared to that calculated through standard mass-luminosity and mass-spectrum relationships. A careful
Externí odkaz:
http://arxiv.org/abs/1609.00487
Publikováno v:
Baltic Astronomy, 24, 367 (2015)
Visual binary stars are the most abundant class of observed binaries. The most comprehensive list of data on visual binaries compiled recently by cross-matching the largest catalogues of visual binaries allowed a statistical investigation of observat
Externí odkaz:
http://arxiv.org/abs/1606.06784
Autor:
Chulkov, D., Prokhorov, M., Malkov, O., Sichevskij, S., Krussanova, N., Mironov, A., Zakharov, A., Kniazev, A.
Publikováno v:
Baltic Astronomy, Vol. 24, p. 137-143 (2015)
The principal goal of this paper is to specify conditions of detection of unresolved binaries by multicolor photometry. We have developed a method for estimating the critical distance at which an unresolved binary of given mass and age can be detecte
Externí odkaz:
http://arxiv.org/abs/1606.01003
Publikováno v:
E3S Web of Conferences, Vol 376, p 01028 (2023)
The article discusses the existing methods of ultrasonic testing of polymer composite materials, reflected in the literature, allowing to determine the size of discontinuities, a method is proposed for determining the depth of folds of fiberglass pro
Externí odkaz:
https://doaj.org/article/8a6722bab8ef473a8d3d922407c06967
Autor:
Malkov O., Kovaleva D., Yungelson L., Avvakumova E., Chulkov D., Dluzhnevskaya O., Kniazev A.
Publikováno v:
Open Astronomy, Vol 25, Iss 4, Pp 384-392 (2016)
We present the results of Monte Carlo simulation aiming to estimate the frequency of semi-detached Algol-type binaries among the stars observed as single. When an account is taken of various detection biases (mostly due to inclination of orbits), the
Externí odkaz:
https://doaj.org/article/c1a205c37e0c42028a7e335334657b82
Publikováno v:
Open Astronomy, Vol 25, Iss 4, Pp 419-426 (2016)
Statistics of orbital parameters of binary stars as well as statistics of their physical characteristics bear traces of star formation history. However, statistical investigations of binaries are complicated by incomplete or missing observational dat
Externí odkaz:
https://doaj.org/article/c9c7f810df95488ea6f752868c7d2ffe
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