No supernovae associated with two long-duration γ-ray bursts

被引：404

作者：

Fynbo, Johan P. U.

Watson, Darach

Thone, Christina C.

Sollerman, Jesper

Bloom, Joshua S.

Davis, Tamara M.

Hjorth, Jens

Jakobsson, Pall

Jorgensen, Uffe G.

Graham, John F.

Fruchter, Andrew S.

Bersier, David

Kewley, Lisa

Cassan, Arnaud

Ceron, Jose Maria Castro

Foley, Suzanne

Gorosabel, Javier

Hinse, Tobias C.

Horne, Keith D.

Jensen, Brian L.

Klose, Sylvio

Kocevski, Daniel

Marquette, Jean-Baptiste

Perley, Daniel

Ramirez-Ruiz, Enrico

Stritzinger, Maximilian D.

Vreeswijk, Paul M.

Wijers, Ralph A. M.

Woller, Kristian G.

Xu, Dong

Zub, Marta

机构：

[1] Univ Copenhagen, Dark Cosmol Ctr, DK-2100 Copenhagen, Denmark

[2] Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen, Denmark

[3] Univ Stockholm, AlbaNova, Dept Astron, S-10691 Stockholm, Sweden

[4] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

[5] Univ Hertfordshire, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England

[6] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[7] Liverpool John Moores Univ, Astrophys Res Inst, Birkenhead CH41 1LD, Merseyside, England

[8] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA

[9] Univ Heidelberg ZAH, Zentrum AStron, ARI, D-69120 Heidelberg, Germany

[10] Univ Coll Dublin, Sch Phys, Dublin 4, Ireland

[11] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain

[12] Univ St Andrews, SUPA Phys Astron, St Andrews KY16 9SS, Fife, Scotland

[13] Thuringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany

[14] Univ Paris 06, CNRS, UMR 70951, Inst Astrophys Paris, F-75014 Paris, France

[15] Inst Adv Study, Princeton, NJ 08540 USA

[16] Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA

[17] Univ Chile, Dept Astron, Santiago, Chile

[18] Univ Amsterdam, Astron Inst Anton Pannekoek, Fac Sci, NL-1098 SJ Amsterdam, Netherlands

来源：

NATURE | 2006年 / 444卷 / 7122期

关键词：

EMISSION; COLLAPSE; LIGHT; DISKS; HST;

D O I：

10.1038/nature05375

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

It is now accepted that long-duration gamma-ray bursts (GRBs) are produced during the collapse of a massive star(1,2). The standard 'collapsar' model(3) predicts that a broad-lined and luminous type Ic core-collapse supernova accompanies every long- duration GRB(4). This association has been confirmed in observations of several nearby GRBs(5-9). Here we report that GRB 060505 ( ref. 10) and GRB 060614 ( ref. 11) were not accompanied by supernova emission down to limits hundreds of times fainter than the archetypal supernova SN 1998bw that accompanied GRB 980425, and fainter than any type Ic supernova ever observed(12). Multi-band observations of the early afterglows, as well as spectroscopy of the host galaxies, exclude the possibility of significant dust obscuration and show that the bursts originated in actively star-forming regions. The absence of a supernova to such deep limits is qualitatively different from all previous nearby long- duration GRBs and suggests a new phenomenological type of massive stellar death.

引用

页码：1047 / 1049

页数：3

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