Free Access
Issue |
Astron. Astrophys. Suppl. Ser.
Volume 138, Number 3, September 1999
Gamma-Ray Bursts in the Afterglow Era Contents Rome, November 3-6, 1998
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Page(s) | 507 - 508 | |
DOI | https://doi.org/10.1051/aas:1999328 | |
Published online | 15 September 1999 |
Astron. Astrophys. Suppl. Ser. 138, 507-508 (1999)
On the nature of GRB-SGRs blazing jets
Physics Dept. Rome, Univ. 1, INFN, Rome, Ple A. Moro 2, Italy
Received:
10
June
1999
Accepted:
30
July
1999
Gamma Ray Burst and Soft Gamma Repeaters are neither standard
candle nor isotropic explosions. Our model explains them as strong
blazing of a light-house, spinning and precessing gamma jet. Such
jets at maximal output (as GRBs in Supernova like sources at
cosmic edges) or at late lower power stages (SGRs in
nearer
planetary nebulae in galactic halo) may blaze the observer by
extreme beaming and apparent huge
luminosity.
Key words: GRB, Jet, Inverse Compton, SGR
© European Southern Observatory (ESO), 1999