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

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Mazzali,  P. A.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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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.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0023-EEE8-2
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