All-Sky Survey in X-Ray
- Autores: Burenin R.A1
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Afiliações:
- Space Research Institute, Russian Academy of Sciences
- Edição: Nº 4 (2022)
- Páginas: 10-16
- Seção: Articles
- URL: https://journals.eco-vector.com/0044-3948/article/view/628491
- DOI: https://doi.org/10.7868/S0044394822040028
- ID: 628491
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Resumo
For the first time ever X-ray optics of Mikhail Pavlinsky ART-XC telescope makes possible the surveys of large areas of the sky in hard X-rays, with the sensitivity maximum at about 10 keV. The main goal of such surveys is studies of various astrophysical objects, whose soft X-ray emission is prone to absorption. Among them are active galactic nuclei, massive X-ray binaries, and cataclysmic variables in our Galaxy.
Bibliografia
- Сюняев Р.А., Арефьев В., Бабышкин В. и др. (Sunyaev R., Arefiev V., Babyshkin V. et al.), Astronomy & Astrophysics, 2021, 656, A132;
- Павлинский М.Н., Ткаченко А., Левин В. и др. (Pavlinsky M., Tkachenko A., Levin V. et al.), Astronomy & Astrophysics, 2021, 650, A42;
- Павлинский М.Н., Сазонов С.Ю., Буренин Р.А. и др. (Pavlinsky M.N., Sazonov S.Yu., Burenin R.A. et al.), Astronomy & Astrophysics, 2022, 661, A38.
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