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  An upper limit to the energy of gamma-ray bursts indicates that GRBs/SNe are powered by magnetars

Mazzali, P. A., McFadyen, A. I., Woosley, S. E., Pian, E., & Tanaka, M. (2014). An upper limit to the energy of gamma-ray bursts indicates that GRBs/SNe are powered by magnetars. Monthly Notices of the Royal Astronomical Society, 443(1), 67-71. doi:10.1093/mnras/stu1124.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0023-EEE8-2 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0023-EEE9-F
Genre: Journal Article

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 Creators:
Mazzali, P. A.1, Author              
McFadyen, A. I., Author
Woosley, S. E., Author
Pian, E., Author
Tanaka, M., Author
Affiliations:
1Stellar Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159882              

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Language(s): eng - English
 Dates: 2014-09-01
 Publication Status: Published in print
 Pages: -
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 Table of Contents: -
 Rev. Method: Peer
 Identifiers: DOI: 10.1093/mnras/stu1124
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Title: Monthly Notices of the Royal Astronomical Society
  Abbreviation : Mon. Not. R. Astr. Soc.
Source Genre: Journal
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Pages: - Volume / Issue: 443 (1) Sequence Number: - Start / End Page: 67 - 71 Identifier: ISSN: 0035-8711
ISSN: 1365-2966