The unusual afterglow of the γ-ray burst of 26 March 1998 as evidence for a supernova connection
Kulkarni, S. R. ; Djorgovski, S. G. ; Eichelberger, A. C. ; Côté, P. ; Blakeslee, J. P. ; Odewahn, S. C. ; Harrison, F. A. ; Frail, D. A. ; Filippenko, A. V. ; Leonard, D. C. ; Riess, A. G. ; Spinrad, H. ; Stern, D. ; Bunker, A. ; Dey, A. ; Grossan, B. ; Perlmutter, S. ; Knop, R. A. ; Hook, I. M. ; Feroci, M. ; Bloom, J. S.
[s.l.] : Macmillian Magazines Ltd.
Published 1999
[s.l.] : Macmillian Magazines Ltd.
Published 1999
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] Cosmic γ-ray bursts have now been firmly established as one of the most powerful phenomena in the Universe, releasing almost the rest-mass energy of a neutron star within the space of a few seconds (ref. 1). The two most popular models to explain γ-ray bursts are ...
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Type of Medium: |
Electronic Resource
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URL: |