Inverse-Compton cooling in Klein-Nishina regime and gamma-ray burst prompt spectrum-Reference-Cited by-同舟云学术

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Inverse-Compton cooling in Klein-Nishina regime and gamma-ray burst prompt spectrum

Published:2012-07-23 Issue:4 Volume:424 Page:3192-3200
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Barniol Duran R.¹,Bošnjak Ž.²,Kumar P.³

Affiliation:

1. Racah Institute of Physics; Edmund J. Safra Campus; Hebrew University of Jerusalem; Jerusalem; 91904; Israel

2. AIM (UMR 7158 CEA/DSM-CNRS-Université Paris Diderot) Irfu/Service d’Astrophysique; Saclay; 91191; Gif-sur-Yvette Cedex; France

3. Department of Astronomy; University of Texas at Austin; Austin; TX; 78712; USA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/424/4/3192/18716115/424-4-3192.pdf

Reference46 articles.

1. Fermi Observations of High-Energy Gamma-Ray Emission from GRB 080916C

2. GeV Emission from Prompt and Afterglow Phases of Gamma‐Ray Bursts

3. SLOW HEATING MODEL OF GAMMA-RAY BURST: PHOTON SPECTRUM AND DELAYED EMISSION

4. Evidence for mild deviation from power-law distribution of electrons in relativistic shocks: GRB 090902B

5. Collisional mechanism for gamma-ray burst emission

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3. Multiwavelength radiation models for low-luminosity GRBs and the implications for UHECRs;Monthly Notices of the Royal Astronomical Society;2022-02-17

4. GRB Afterglow Parameters in the Era of TeV Observations: The Case of GRB 190114C;The Astrophysical Journal;2021-12-01

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