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

Chris L. Fryer; Paolo A. Mazzali; Jason Prochaska; Enrico Cappellaro; Alin Panaitescu; Edo Berger; Maurice Van Putten; Ed P J Van Den Heuvel; Patrick Young; Aimee Hungerford; Gabriel Rockefeller; Sung Chul Yoon; Philipp Podsiadlowski; Ken'ichi Nomoto; Roger Chevalier; Brian Schmidt; Shri Kulkarni

doi:10.1086/523768

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

Chris L. Fryer, Paolo A. Mazzali, Jason Prochaska, Enrico Cappellaro, Alin Panaitescu, Edo Berger, Maurice Van Putten, Ed P J Van Den Heuvel, Patrick Young, Aimee Hungerford, Gabriel Rockefeller, Sung Chul Yoon, Philipp Podsiadlowski, Ken'ichi Nomoto, Roger Chevalier, Brian Schmidt, Shri Kulkarni

Earth and Space Exploration, School of (SESE)

Research output: Contribution to journal › Review article › peer-review

102 Scopus citations

Abstract

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.

Original language	English (US)
Pages (from-to)	1211-1232
Number of pages	22
Journal	Publications of the Astronomical Society of the Pacific
Volume	119
Issue number	861
DOIs	https://doi.org/10.1086/523768
State	Published - Nov 2007

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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Fryer, C. L., Mazzali, P. A., Prochaska, J., Cappellaro, E., Panaitescu, A., Berger, E., Van Putten, M., Van Den Heuvel, E. P. J., Young, P., Hungerford, A., Rockefeller, G., Yoon, S. C., Podsiadlowski, P., Nomoto, K., Chevalier, R., Schmidt, B., & Kulkarni, S. (2007). Constraints on type Ib/c supernovae and gamma-ray burst progenitors. Publications of the Astronomical Society of the Pacific, 119(861), 1211-1232. https://doi.org/10.1086/523768

Fryer, CL, Mazzali, PA, Prochaska, J, Cappellaro, E, Panaitescu, A, Berger, E, Van Putten, M, Van Den Heuvel, EPJ, Young, P, Hungerford, A, Rockefeller, G, Yoon, SC, Podsiadlowski, P, Nomoto, K, Chevalier, R, Schmidt, B & Kulkarni, S 2007, 'Constraints on type Ib/c supernovae and gamma-ray burst progenitors', Publications of the Astronomical Society of the Pacific, vol. 119, no. 861, pp. 1211-1232. https://doi.org/10.1086/523768

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title = "Constraints on type Ib/c supernovae and gamma-ray burst progenitors",

abstract = "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.",

author = "Fryer, {Chris L.} and Mazzali, {Paolo A.} and Jason Prochaska and Enrico Cappellaro and Alin Panaitescu and Edo Berger and {Van Putten}, Maurice and {Van Den Heuvel}, {Ed P J} and Patrick Young and Aimee Hungerford and Gabriel Rockefeller and Yoon, {Sung Chul} and Philipp Podsiadlowski and Ken'ichi Nomoto and Roger Chevalier and Brian Schmidt and Shri Kulkarni",

year = "2007",

month = nov,

doi = "10.1086/523768",

language = "English (US)",

volume = "119",

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AU - Fryer, Chris L.

AU - Mazzali, Paolo A.

AU - Prochaska, Jason

AU - Cappellaro, Enrico

AU - Panaitescu, Alin

AU - Berger, Edo

AU - Van Putten, Maurice

AU - Van Den Heuvel, Ed P J

AU - Young, Patrick

AU - Hungerford, Aimee

AU - Rockefeller, Gabriel

AU - Yoon, Sung Chul

AU - Podsiadlowski, Philipp

AU - Nomoto, Ken'ichi

AU - Chevalier, Roger

AU - Schmidt, Brian

AU - Kulkarni, Shri

PY - 2007/11

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N2 - 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.

AB - 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.

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

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