Constraints on type Ib/c supernovae and gamma-ray burst progenitors

被引：101

作者：

Fryer, Chris L. ^{[1
,2
]}

Mazzali, Paolo A. ^{[3
,4
]}

Prochaska, Jason ^{[5
]}

Cappellaro, Enrico ^{[6
]}

Panaitescu, Alin ^{[7
]}

Berger, Edo ^{[8
,9
]}

Van Putten, Maurice ^{[10
]}

van den Heuvel, Ed P. J. ^{[11
]}

Young, Patrick ^{[12
,13
]}

Hungerford, Aimee ^{[2
]}

Rockefeller, Gabriel ^{[2
]}

Yoon, Sung-Chul ^{[11
]}

Podsiadlowski, Philipp ^{[14
]}

Nomoto, Ken'ichi ^{[15
]}

Chevalier, Roger ^{[16
]}

Schmidt, Brian ^{[17
]}

Kulkarni, Shri ^{[18
]}

机构：

[1] Univ Arizona, Dept Phys, Tucson, AZ 85721 USA

[2] Stat Sci Div, Los Alamos Natl Lab, Los Alamos, NM USA

[3] Osserv Astron Trieste, INAF, Trieste, Italy

[4] Max Planck Inst Astrophys, Garching, Germany

[5] Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA USA

[6] Osserv Astron Padova, INAF, Padua, Italy

[7] Integrated Spectroscopy Resource Div, Los Alamos Natl Lab, Los Alamos, NM USA

[8] Observ Carnegie Inst Washington, Pasadena, CA USA

[9] Princeton Univ Observ, Princeton, NJ USA

[10] MIT, Laser Interferometer Gravit Wave Observ Lab, Cambridge, MA USA

[11] Univ Amsterdam, Astron Inst Anton Pannekoek, Amsterdam, Netherlands

[12] Univ Arizona, Dept Astron, Tucson, AZ USA

[13] Div Appl Phys, Los Alamos Natl Lab, Los Alamos, NM USA

[14] Univ Oxford, Dept Astrophys, Oxford OX1 2JD, England

[15] Univ Tokyo, Dept Astron, RESCUE, Bunkyo Ku, Tokyo, Japan

[16] Univ Virginia, Dept Astron, Charlottesville, VA USA

[17] Mt Stromlo & Siding Spring Observ, Canberra, ACT, Australia

[18] CALTECH, Caltech Opt Observ, Pasadena, CA USA

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 2007年 / 119卷 / 861期

关键词：

D O I：

10.1086/523768

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Although there is strong support for the collapsar engine as the power source of long-duration gamma-ray bursts (GRBs), we still do not definitively know the progenitor of these explosions. Here we review the current set of progenitor scenarios for long-duration GRBs and the observational constraints on these scenarios. Examining these models, we find that single stars cannot be the only progenitor for long-duration GRBs. Several binary progenitors can match the solid observational constraints and also have the potential to match the trends that we are currently seeing in the observations. Type Ib/c supernovae are also likely to be produced primarily in binaries; we discuss the relationship between the progenitors of these explosions and those of the long-duration GRBs.

引用

页码：1211 / 1232

页数：22

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