Off-axis Afterglow Closure Relations and Fermi-LAT Detected Gamma-Ray Bursts

被引：0

作者：

Fraija, N. ^{[1
]}

Dainotti, M.G. ^{[2
,3
,4
]}

Levine, D. ^{[5
]}

Betancourt Kamenetskaia, B. ^{[6
,7
]}

Galvan-Gamez, A. ^{[1
]}

机构：

[1] Instituto de Astronomía, Universidad Nacional Autónoma de México, Circuito Exterior, C.U., A. Postal 70-264, México City,04510, Mexico

[2] National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo,181-8588, Japan

[3] Space Science Institute, Boulder,CO, United States

[4] The Graduate University for Advanced Studies, SOKENDAI, Shonankokusaimura, Hayama, Miura District, Kanagawa,240-0193, Japan

[5] Department of Astronomy, University of Maryland, College Park,MD,20742, United States

[6] Technical University of Munich, TUM School of Natural Sciences, Physics Department, James-Franck-Str 1, Garching,85748, Germany

[7] Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), Föhringer Ring 6, Munich,80805, Germany

来源：

arXiv | 2023年

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摘要：

Acceleration - Gamma rays - Germanium alloys - Germanium compounds - Stars

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