An unexpectedly rapid decline in the X-ray afterglow emission of long γ-ray bursts
Goad, M. ; Chincarini, G. ; Moretti, A. ; Campana, S. ; Burrows, D. N. ; Perri, M. ; Barthelmy, S. D. ; Gehrels, N. ; Krimm, H. ; Sakamoto, T. ; Kumar, P. ; Mészáros, P. I. ; Kobayashi, S. ; Zhang, B. ; Angelini, L. ; Banat, P. ; Beardmore, A. P. ; Capalbi, M. ; Covino, S. ; Cusumano, G. ; Giommi, P. ; Godet, O. ; Hill, J. E. ; Kennea, J. A. ; Mangano, V.
[s.l.] : Nature Publishing Group
Published 2005
[s.l.] : Nature Publishing Group
Published 2005
| ISSN: |
1476-4687
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|---|---|
| Source: |
Nature Archives 1869 - 2009
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| Topics: |
Biology
Chemistry and Pharmacology
Medicine
Natural Sciences in General
Physics
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| Notes: |
[Auszug] ‘Long’ γ-ray bursts (GRBs) are commonly accepted to originate in the explosion of particularly massive stars, which give rise to highly relativistic jets. Inhomogeneities in the expanding flow result in internal shock waves that are believed to produce the γ-rays we see. ...
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| Type of Medium: |
Electronic Resource
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| URL: |