Identifying objects of the optical range in the regions of hard radiation near red dwarf stars

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Published: 30.09.2024
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Aleksei Shlyapnikov
Crimean Astrophysical Observatory, Nauchny 298409

Abstract

We analyze the localization regions of TeV gamma-ray sources in the X-ray and optical spectral ranges. The angle distances from the position of maxima in the distribution of high-energy fluxes to the probable candidates for identification with red dwarfs are indicated. Possible identifications of fainter TeV sources and other field objects are also considered.

Keywords: X-ray and gamma-ray sources, stars – variable and peculiar

Supporting Agencies

The author is grateful to all who ensure their operation and expresses gratitude to the Russian Foundation for Basic Research for partial support of the conducted research through grants No. 19-02-00191 and No. 19-29-11027.

Article Details

Issue

Vol. 5 No. 3 (2024)

Section

Magnetism and activity of the Sun and stars – 2021 Conference proceedings

How to Cite

Shlyapnikov A., 2024. Acta Astrophysica Taurica, vol. 5, no. 3, pp. 18–26. Available at: https://astrophysicatauricum.org/index.php/aat/article/view/85 (Accessed: 21 March 2026)

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