Studying the SN-GRB connection with X-shooter: The GRB 100316D/SN2010bh case

被引：9

作者：

Bufano, F. ^{[1
]}

Benetti, S. ^{[2
]}

Sollerman, J. ^{[3
]}

Pian, E. ^{[4
,5
]}

Cupani, G. ^{[4
]}

机构：

[1] Osserv Astrofis Catania, INAF, I-95123 Catania, Italy

[2] Osserv Astron Padova, INAF, I-35122 Padua, Italy

[3] Oskar Klein Ctr, Dept Astron, SE-10691 Stockholm, Sweden

[4] Osserv Astron Trieste, INAF, I-34143 Trieste, Italy

[5] Scuola Normale Super Pisa, I-56126 Pisa, Italy

来源：

ASTRONOMISCHE NACHRICHTEN | 2011年 / 332卷 / 03期

关键词：

gamma rays: bursts; supernovae: general; supernovae: individual (SN2010bh); GAMMA-RAY BURST; 25; APRIL; 1998; NEUTRON-STAR; SUPERNOVA; GRB-060218; EVOLUTION; MODELS;

D O I：

10.1002/asna.201111531

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

During the last ten years, observations of long-duration gamma-ray bursts brought to the conclusion that at least a fraction of them is associated with bright supernovae of type Ib/c. In this talk, after a short review on the previously observed GRB-SN connection cases, we present the recent case of GRB 100316/SN 2010bh. In particular, during the observational campaign of SN 2010bh, a pivotal role was played by VLT/X-shooter, sampling with unique high quality data the spectral energy distribution of the early evolution phases from the UV to the K band. (C) 2011 WILEY-VCH Verlag GmbH&Co. KGaA, Weinheim

引用

页码：262 / 265

页数：4

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