On the possible association of SN 1998bw and GRB 980425

被引：46

作者：

Galama, TJ

Vreeswijk, PM

van Paradijs, J

Kouveliotou, C

Augusteijn, T

Patat, F

Heise, J

't Zand, JI

Groot, PJ

Wijers, RAMJ

Pian, E

Palazzi, E

Frontera, F

Masetti, N

机构：

[1] Univ Amsterdam, Astron Inst Anton Pannekoek, CHEAF, NL-1098 SJ Amsterdam, Netherlands

[2] UAH, Dept Phys, Huntsville, AL 35899 USA

[3] Univ Space Res Assoc, Washington, DC USA

[4] NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA

[5] ESO, Santiago 19, Chile

[6] SRON, Space Res Lab, NL-3584 CA Utrecht, Netherlands

[7] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA

[8] CNR, Ist Tecnol & Studio Radiaz Extraterr, Bologna, Italy

来源：

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1999年 / 138卷 / 03期

关键词：

gamma-rays : bursts; (stars :) supernovae : individual : SN 1998bw;

D O I：

10.1051/aas:1999311

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We here discuss the possibility that the peculiar supernova SN 1998bw and the Gamma-Ray Burst GRB 980425 are associated. If the two are related, the energy radiated in gamma rays is at least four orders of magnitude less than in other GRBs, although its appearance is otherwise unremarkable: this suggests that very different mechanisms may give rise to GRBs.

引用

页码：465 / 466

页数：2

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