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The spatiotemporal coincidence of supernova (SN) 1998bw and gamma-ray burst (GRB) 980425 and this supernova's unusual optical and radio properties have prompted many theoretical models that produce GRBs from supernovae. We review the…

天体物理学 · 物理学 2009-11-06 Jonathan C. Tan , Christopher D. Matzner , Christopher F. McKee

The discovery of a supernova emerging at late times in the afterglow of GRB 030329 has apparently settled the issue on the nature of the progenitor of gamma-ray bursts. We now know that at least a fraction of cosmological GRBs are…

天体物理学 · 物理学 2016-11-09 Davide Lazzati

Since 1997 the afterglow of gamma-ray bursting sources (GRBs) has occasionally been detected in the radio, as well in other wavelengths bands. In particular, the interesting and unusual gamma-ray burst GRB980425, thought to be related to…

天体物理学 · 物理学 2016-04-13 Kurt W. Weiler , Nino Panagia , Marcos J. Montes

The recent discovery of the unusual supernova SN1998bw and its apparent correlation with the gamma-ray burst GRB 980425 has raised new issues concerning both the GRB and SNe. SN1998bw was unusually bright at maximum light and expansion…

天体物理学 · 物理学 2007-05-23 P. Hoeflich , J. C. Wheeler , L. Wang

There are hints that nearby Type Ia supernovae may be a little different than those at large redshift. Confidence in the conclusion that there is a cosmological constant and an accelerating Universe thus still requires the hard work of…

天体物理学 · 物理学 2007-05-23 J. Craig Wheeler

Over the six years since the discovery of the gamma-ray burst GRB 980425, associated with the nearby (distance, ~40 Mpc) supernova 1998bw, astronomers have fiercely debated the nature of this event. Relative to bursts located at…

SN 1998bw is an unusual Type Ic supernova that may be associated with the $\gamma$-ray burst GRB 980425. We use a synchrotron self-absorption model for its radio emission to deduce that the synchrotron-emitting gas is expanding into a…

天体物理学 · 物理学 2009-10-31 Zhi-Yun Li , Roger A. Chevalier

The unusual supernova SN1998bw, which is thought to be related to the gamma-ray burster GRB980425, is a possible link between the two classes of objects. Analyzing the extensive radio emission data avaliable for SN1998bw, we are able to…

天体物理学 · 物理学 2009-11-06 Kurt W. Weiler , Nino Panagia , Marcos J. Montes

The spatial and temporal coincidence between the gamma-ray burst (GRB) 980425 and supernova (SN) 1998bw has prompted speculation that there exists a class of GRBs produced by SNe (``S-GRBs''). Robust arguments for the existence of a…

天体物理学 · 物理学 2009-10-30 J. S. Bloom , S. R. Kulkarni , F. Harrison , T. Prince , E. S. Phinney , D. A. Frail

Recently a Type Ic supernova, SN 1998bw, was discovered coincident with a gamma-ray burst, GRB 980425. The supernova had unusual radio, optical, and spectroscopic properties. We explore here models based upon helium stars in the range 9 -…

天体物理学 · 物理学 2009-10-30 S. E. Woosley , Ronald G. Eastman , Brian P. Schmidt

The recent discovery of the unusual supernova SN1998bw and its apparent correlation with the gamma-ray burst GRB 980425 has raised new issues concerning both the GRB and supernovae. Although the spectra resemble those of TypeIc supernovae,…

天体物理学 · 物理学 2009-10-30 P. Hoeflich , J. C. Wheeler , L. Wang

Some gamma ray bursts may be produced by supernovae exploding in close massive binary systems (type Ib/c supernovae) as suggested by the recent observation of SN 1998bw/GRB 980425. We propose that high energy radiation observed in such…

天体物理学 · 物理学 2007-05-23 R. J. Protheroe , W. Bednarek

The advent of large panoramic photometric surveys of the sky offers the possibly of exploring the association of gamma-ray bursts (GRBs) with supernovae. To date, a few gamma-ray bursts have been connected possibly with supernovae: GRB…

天体物理学 · 物理学 2009-11-07 Jeremy S. Heyl

Cosmic gamma-ray bursts (GRBs) have been firmly established as one of the most powerful phenomena in the Universe, releasing electromagnetic energy approaching the rest-mass energy of a neutron star in a few seconds. The two currently…

SN1998bw shot to fame by claims of association with GRB980425. Independent of its presumed association with a GRB, this SN is unusual in its radio properties. A simple interpretation of the unusually bright radio emission leads us to the…

天体物理学 · 物理学 2009-10-31 M. H. Wieringa , S. R. Kulkarni , D. A. Frail

Supernova SN 1998bw exploded in the same direction and at the same time as the gamma-ray burst GRB 980425. Here we report radio observations of this type Ic supernova, beginning 4 days after the gamma-ray burst. At its peak the radio source…

The gamma ray burst (GRB) 980425 is distinctive in that it seems to be associated with supernova (SN) 1998bw, has no X-ray afterglow, and has a single peak light curve and a soft spectrum. The supernova is itself unusual in that its…

天体物理学 · 物理学 2009-10-31 D. Eichler , A. Levinson

The late-time high-resolution X-ray and radio observations of GRB980425/SN1998bw, the closest known gamma ray burst (GRB) associated with a supernova (SN) explosion, may have actually resolved the hyperluminal source that produced the GRB…

高能天体物理现象 · 物理学 2016-10-11 Shlomo Dado , Arnon Dar , A. De Rujula

We use the very simple and successful Cannonball Model (CB) of gamma ray bursts (GRBs) and their afterglows (AGs) to analyze the observations of the strongly extinct optical AG of GRB 010921 with ground-based telescopes at early times, and…

天体物理学 · 物理学 2007-05-23 Shlomo Dado , Arnon Dar , Alvaro De Rujula

Study of the polarization of supernovae has suggested that the core collapse process may be intrinsically strongly asymmetric. There is a tentative trend for supernova with smaller envelopes showing more polarization, with Type Ic having…

天体物理学 · 物理学 2007-05-23 J. Craig Wheeler , Peter Hoeflich , Lifan Wang
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