Search for correlations between BATSE gamma-ray bursts and supernovae

被引：1

作者：

Polcar, J. ^{[1
]}

Topinka, M.

Necas, D.

Hudec, R.

Hudcova, V.

Hroch, F.

Masetti, N.

Pizzichini, G.

Palazzi, E.

机构：

[1] Acad Sci Czech Republ, Inst Astron, CS-25165 Ondrejov, Czech Republic

[2] Masaryk Univ, Fac Sci, CS-61137 Brno, Czech Republic

[3] Max Planck Inst Astrophys, D-85741 Garching, Germany

[4] Brno Univ Technol, Fac Civil Engn, Brno, Czech Republic

[5] Inst Astrofis Spaziale & Fis Cosm, INAF, Sez Bologna, I-40129 Bologna, Italy

来源：

ASTRONOMY & ASTROPHYSICS | 2006年 / 452卷 / 02期

关键词：

gamma rays : bursts; stars : supernovae : general; methods : statistical;

D O I：

10.1051/0004-6361:20053584

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report on our statistical research of space-time correlated supernovae and CGRO-BATSE gamma-ray bursts. There exists a significantly higher abundance of core-collapse supernovae among the correlated supernovae, but the subset of all correlated objects does not seem to be physically different from the whole set. The upper limit of the fraction of possibly correlated GRBs and SNe is of order of a few percent.

引用

页码：439 / 449

页数：11

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