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Reverse Shock Emission in Gamma-Ray Bursts Revisited
Joint Authors
Source
Issue
Vol. 2015, Issue 2015 (31 Dec. 2015), pp.1-16, 16 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2015-08-24
Country of Publication
Egypt
No. of Pages
16
Main Subjects
Abstract EN
A generic synchrotron external shock model is the widely preferred paradigm used to interpret the broadband afterglow data of gamma-ray bursts (GRBs), including predicted observable signatures from areverse shock which have been confirmed by observations.
Investigations of the nature of the reverse shock emission can provide valuable insights into the intrinsic properties of the GRB ejecta.
Here we briefly review the standard and the extended models of the reverse shock emission, discussing the connection between the theory and observations, including the implications of the latest observational advances.
American Psychological Association (APA)
Gao, He& Mészáros, Peter. 2015. Reverse Shock Emission in Gamma-Ray Bursts Revisited. Advances in Astronomy،Vol. 2015, no. 2015, pp.1-16.
https://search.emarefa.net/detail/BIM-1051959
Modern Language Association (MLA)
Gao, He& Mészáros, Peter. Reverse Shock Emission in Gamma-Ray Bursts Revisited. Advances in Astronomy No. 2015 (2015), pp.1-16.
https://search.emarefa.net/detail/BIM-1051959
American Medical Association (AMA)
Gao, He& Mészáros, Peter. Reverse Shock Emission in Gamma-Ray Bursts Revisited. Advances in Astronomy. 2015. Vol. 2015, no. 2015, pp.1-16.
https://search.emarefa.net/detail/BIM-1051959
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-1051959