Does regenerated emission change the high-energy signal from gamma-ray burst afterglows?
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/354/2/414/3870569/354-2-414.pdf
Reference41 articles.
Cited by 10 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Modelling synchrotron and synchrotron self-Compton emission of gamma-ray burst afterglows from radio to very-high energies;Monthly Notices of the Royal Astronomical Society;2021-05-10
2. CONTRIBUTION OF GAMMA-RAY-LOUD RADIO GALAXIES’ CORE EMISSIONS TO THE COSMIC MeV AND GeV GAMMA-RAY BACKGROUND RADIATION;The Astrophysical Journal;2011-05-05
3. HIGH ENERGY GAMMA-RAY ABSORPTION AND CASCADE EMISSION IN NEARBY STARBURST GALAXIES;The Astrophysical Journal;2011-01-13
4. EVIDENCE FOR GAMMA-RAY HALOS AROUND ACTIVE GALACTIC NUCLEI AND THE FIRST MEASUREMENT OF INTERGALACTIC MAGNETIC FIELDS;The Astrophysical Journal;2010-09-17
5. Possible effects of pair echoes on gamma-ray burst afterglow emission;Monthly Notices of the Royal Astronomical Society;2009-07-11
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