A relativistic type Ibc supernova without a detected γ-ray burst.
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| Title: | A relativistic type Ibc supernova without a detected γ-ray burst. |
|---|---|
| Authors: | Soderberg, A. M., Chakraborti, S., Pignata, G., Chevalier, R. A., Chandra, P., Ray, A., Wieringa, M. H., Copete, A., Chaplin, V., Connaughton, V., Barthelmy, S. D., Bietenholz, M. F., Chugai, N., Stritzinger, M. D., Hamuy, M., Fransson, C., Fox, O., Levesque, E. M., Grindlay, J. E., Challis, P. |
| Source: | Nature. 1/28/2010, Vol. 463 Issue 7280, p513-515. 3p. 4 Graphs. |
| Subjects: | Type I supernovae, Neutron stars, Solar radio emission, Satellite dish antennas, Engines, Astrophysical collisions, Particles (Nuclear physics), Pulsars, Physical sciences |
| Abstract: | Long duration γ-ray bursts (GRBs) mark the explosive death of some massive stars and are a rare sub-class of type Ibc supernovae. They are distinguished by the production of an energetic and collimated relativistic outflow powered by a central engine (an accreting black hole or neutron star). Observationally, this outflow is manifested in the pulse of γ-rays and a long-lived radio afterglow. Until now, central-engine-driven supernovae have been discovered exclusively through their γ-ray emission, yet it is expected that a larger population goes undetected because of limited satellite sensitivity or beaming of the collimated emission away from our line of sight. In this framework, the recovery of undetected GRBs may be possible through radio searches for type Ibc supernovae with relativistic outflows. Here we report the discovery of luminous radio emission from the seemingly ordinary type Ibc SN 2009bb, which requires a substantial relativistic outflow powered by a central engine. A comparison with our radio survey of type Ibc supernovae reveals that the fraction harbouring central engines is low, about one per cent, measured independently from, but consistent with, the inferred rate of nearby GRBs. Independently, a second mildly relativistic supernova has been reported. [ABSTRACT FROM AUTHOR] |
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| Database: | Psychology and Behavioral Sciences Collection |
| FullText | Links: – Type: pdflink Text: Availability: 0 |
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| Header | DbId: pbh DbLabel: Psychology and Behavioral Sciences Collection An: 47754078 AccessLevel: 6 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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H.</searchLink><br /><searchLink fieldCode="AR" term="%22Copete%2C+A%2E%22">Copete, A.</searchLink><br /><searchLink fieldCode="AR" term="%22Chaplin%2C+V%2E%22">Chaplin, V.</searchLink><br /><searchLink fieldCode="AR" term="%22Connaughton%2C+V%2E%22">Connaughton, V.</searchLink><br /><searchLink fieldCode="AR" term="%22Barthelmy%2C+S%2E+D%2E%22">Barthelmy, S. D.</searchLink><br /><searchLink fieldCode="AR" term="%22Bietenholz%2C+M%2E+F%2E%22">Bietenholz, M. F.</searchLink><br /><searchLink fieldCode="AR" term="%22Chugai%2C+N%2E%22">Chugai, N.</searchLink><br /><searchLink fieldCode="AR" term="%22Stritzinger%2C+M%2E+D%2E%22">Stritzinger, M. D.</searchLink><br /><searchLink fieldCode="AR" term="%22Hamuy%2C+M%2E%22">Hamuy, M.</searchLink><br /><searchLink fieldCode="AR" term="%22Fransson%2C+C%2E%22">Fransson, C.</searchLink><br /><searchLink fieldCode="AR" term="%22Fox%2C+O%2E%22">Fox, O.</searchLink><br /><searchLink fieldCode="AR" term="%22Levesque%2C+E%2E+M%2E%22">Levesque, E. M.</searchLink><br /><searchLink fieldCode="AR" term="%22Grindlay%2C+J%2E+E%2E%22">Grindlay, J. E.</searchLink><br /><searchLink fieldCode="AR" term="%22Challis%2C+P%2E%22">Challis, P.</searchLink> – Name: TitleSource Label: Source Group: Src Data: <searchLink fieldCode="JN" term="%22Nature%22">Nature</searchLink>. 1/28/2010, Vol. 463 Issue 7280, p513-515. 3p. 4 Graphs. – Name: Subject Label: Subjects Group: Su Data: <searchLink fieldCode="DE" term="%22Type+I+supernovae%22">Type I supernovae</searchLink><br /><searchLink fieldCode="DE" term="%22Neutron+stars%22">Neutron stars</searchLink><br /><searchLink fieldCode="DE" term="%22Solar+radio+emission%22">Solar radio emission</searchLink><br /><searchLink fieldCode="DE" term="%22Satellite+dish+antennas%22">Satellite dish antennas</searchLink><br /><searchLink fieldCode="DE" term="%22Engines%22">Engines</searchLink><br /><searchLink fieldCode="DE" term="%22Astrophysical+collisions%22">Astrophysical collisions</searchLink><br /><searchLink fieldCode="DE" term="%22Particles+%28Nuclear+physics%29%22">Particles (Nuclear physics)</searchLink><br /><searchLink fieldCode="DE" term="%22Pulsars%22">Pulsars</searchLink><br /><searchLink fieldCode="DE" term="%22Physical+sciences%22">Physical sciences</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: Long duration γ-ray bursts (GRBs) mark the explosive death of some massive stars and are a rare sub-class of type Ibc supernovae. They are distinguished by the production of an energetic and collimated relativistic outflow powered by a central engine (an accreting black hole or neutron star). Observationally, this outflow is manifested in the pulse of γ-rays and a long-lived radio afterglow. Until now, central-engine-driven supernovae have been discovered exclusively through their γ-ray emission, yet it is expected that a larger population goes undetected because of limited satellite sensitivity or beaming of the collimated emission away from our line of sight. In this framework, the recovery of undetected GRBs may be possible through radio searches for type Ibc supernovae with relativistic outflows. Here we report the discovery of luminous radio emission from the seemingly ordinary type Ibc SN 2009bb, which requires a substantial relativistic outflow powered by a central engine. A comparison with our radio survey of type Ibc supernovae reveals that the fraction harbouring central engines is low, about one per cent, measured independently from, but consistent with, the inferred rate of nearby GRBs. Independently, a second mildly relativistic supernova has been reported. [ABSTRACT FROM AUTHOR] – Name: AbstractSuppliedCopyright Label: Group: Ab Data: <i>Copyright of Nature is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.) |
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| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1038/nature08714 Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 3 StartPage: 513 Subjects: – SubjectFull: Type I supernovae Type: general – SubjectFull: Neutron stars Type: general – SubjectFull: Solar radio emission Type: general – SubjectFull: Satellite dish antennas Type: general – SubjectFull: Engines Type: general – SubjectFull: Astrophysical collisions Type: general – SubjectFull: Particles (Nuclear physics) Type: general – SubjectFull: Pulsars Type: general – SubjectFull: Physical sciences Type: general Titles: – TitleFull: A relativistic type Ibc supernova without a detected γ-ray burst. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Soderberg, A. M. – PersonEntity: Name: NameFull: Chakraborti, S. – PersonEntity: Name: NameFull: Pignata, G. – PersonEntity: Name: NameFull: Chevalier, R. A. – PersonEntity: Name: NameFull: Chandra, P. – PersonEntity: Name: NameFull: Ray, A. – PersonEntity: Name: NameFull: Wieringa, M. H. – PersonEntity: Name: NameFull: Copete, A. – PersonEntity: Name: NameFull: Chaplin, V. – PersonEntity: Name: NameFull: Connaughton, V. – PersonEntity: Name: NameFull: Barthelmy, S. D. – PersonEntity: Name: NameFull: Bietenholz, M. F. – PersonEntity: Name: NameFull: Chugai, N. – PersonEntity: Name: NameFull: Stritzinger, M. D. – PersonEntity: Name: NameFull: Hamuy, M. – PersonEntity: Name: NameFull: Fransson, C. – PersonEntity: Name: NameFull: Fox, O. – PersonEntity: Name: NameFull: Levesque, E. M. – PersonEntity: Name: NameFull: Grindlay, J. E. – PersonEntity: Name: NameFull: Challis, P. IsPartOfRelationships: – BibEntity: Dates: – D: 28 M: 01 Text: 1/28/2010 Type: published Y: 2010 Identifiers: – Type: issn-print Value: 00280836 Numbering: – Type: volume Value: 463 – Type: issue Value: 7280 Titles: – TitleFull: Nature Type: main |
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