Zobrazeno 1 - 10
of 13
pro vyhledávání: '"S. G. Sichevskij"'
Publikováno v:
Solar System Research. 53:560-566
This paper presents the project of the space astrophysical observatory Astron-2 aimed to carry out the all-sky spectral and photometric survey in the ultraviolet spectral region (115–310 nm). The major instrument of the observatory is a 210-cm aper
Autor:
S. G. Sichevskij
Publikováno v:
Astrophysical Bulletin. 73:98-107
The feasibility of the determination of the physical conditions in star’s atmosphere and the parameters of interstellar extinction from broad-band photometric observations in the 300–3000 nm wavelength interval is studied using SDSS and 2MASS dat
Autor:
S. G. Sichevskij
Publikováno v:
Astrophysical Bulletin. 72:141-149
We describe Bayesian probabilistic approach to estimating the properties of stars and the interstellar extinction law based on photometric observations and using prior data about the parameters of the stars. The accuracy of the resulting estimates is
Autor:
S. G. Sichevskij
Publikováno v:
Astronomy Reports. 61:193-205
A technique for determining a star’s radius from its atmospheric characteristics (effective temperature, surface gravity, and metallicity) is realized based on modernmodel computations of the stellar internal structure and evolution. The atmospheri
Autor:
S. G. Sichevskij
Publikováno v:
Astrophysical Bulletin. 72:51-57
Based on the spectral observations of the LAMOST (DR2) survey, the radii, masses, and luminosities of 700 481 stars were estimated. These stars belong to spectral types A, F, G, and K, and have metallicities between −0.845 and 0.0. To determine the
Autor:
S. G. Sichevskij
Publikováno v:
Astronomy Reports. 60:816-830
A method for determining the radius of a star based on its effective temperature and surface gravity together with computations of the star’s structure and evolution is proposed. Rotating and nonrotating stellar models are considered, making it pos
Autor:
S. G. Sichevskij
Publikováno v:
Astronomy Reports. 60:598-610
Amethod for determining the radius of a star using its effective temperature and surface gravity is proposed. The method assumes that the relationship between the radius, effective temperature, and surface gravity can be approximated using models for
Publikováno v:
Astrophysical Bulletin. 69:160-168
The development and application of new methods for intelligent analysis and extraction of information from digital sky surveys carried out in various spectral domains have now become a popular field in astrophysical research and, in particular, in st
Publikováno v:
SPIE Proceedings.
The World Space Observatory--Ultraviolet (WSO--UV) is a Russian-Spanish space mission born as a response to the growing up demand for UV facilities by the astronomical community. Main components of the WSO-UV Ground Segment, Mission Control Centre an
Autor:
M. E. Prokhorov, A. Y. Kniazev, S. G. Sichevskij, A. V. Mironov, N. Krussanova, Andrey I. Zakharov, O. Malkov, D. A. Chulkov
Publikováno v:
Open Astronomy, Vol 24, Iss 2, Pp 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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::446f9ddb8313d6a251288b91396d6479
http://arxiv.org/abs/1606.01003
http://arxiv.org/abs/1606.01003