A transient radio source consistent with a merger-triggered core collapse supernova.
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| Title: | A transient radio source consistent with a merger-triggered core collapse supernova. |
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| Authors: | Dong, D. Z., Hallinan, G., Nakar, E., Ho, A. Y. Q., Hughes, A. K., Hotokezaka, K., Myers, S. T., De, K., Mooley, K. P., Ravi, V., Horesh, A., Kasliwal, M. M., Kulkarni, S. R. |
| Source: | Science (pre-March 2025). 9/3/2021, Vol. 373 Issue 6559, p1125-1129. 5p. 4 Graphs. |
| Subjects: | Radio sources (Astronomy), Supernovae, Exothermic reactions, Supergiant stars, Nuclear fuels, Stellar mergers, Very large array telescopes, Radio jets (Astrophysics) |
| Abstract: | A core collapse supernova occurs when exothermic fusion ceases in the core of a massive star, which is typically caused by exhaustion of nuclear fuel. Theory predicts that fusion could be interrupted earlier by merging of the star with a compact binary companion. We report a luminous radio transient, VT J121001+495647, found in the Very Large Array Sky Survey. The radio emission is consistent with supernova ejecta colliding with a dense shell of material, potentially ejected by binary interaction in the centuries before explosion. We associate the supernova with an archival x-ray transient, which implies that a relativistic jet was launched during the explosion. The combination of an early relativistic jet and late-time dense interaction is consistent with expectations for a merger-driven explosion. [ABSTRACT FROM AUTHOR] |
| Copyright of Science (pre-March 2025) is the property of American Association for the Advancement of Science 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. (Copyright applies to all Abstracts.) | |
| 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: 152270803 AccessLevel: 6 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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| Items | – Name: Title Label: Title Group: Ti Data: A transient radio source consistent with a merger-triggered core collapse supernova. – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22Dong%2C+D%2E+Z%2E%22">Dong, D. Z.</searchLink><br /><searchLink fieldCode="AR" term="%22Hallinan%2C+G%2E%22">Hallinan, G.</searchLink><br /><searchLink fieldCode="AR" term="%22Nakar%2C+E%2E%22">Nakar, E.</searchLink><br /><searchLink fieldCode="AR" term="%22Ho%2C+A%2E+Y%2E+Q%2E%22">Ho, A. Y. Q.</searchLink><br /><searchLink fieldCode="AR" term="%22Hughes%2C+A%2E+K%2E%22">Hughes, A. K.</searchLink><br /><searchLink fieldCode="AR" term="%22Hotokezaka%2C+K%2E%22">Hotokezaka, K.</searchLink><br /><searchLink fieldCode="AR" term="%22Myers%2C+S%2E+T%2E%22">Myers, S. T.</searchLink><br /><searchLink fieldCode="AR" term="%22De%2C+K%2E%22">De, K.</searchLink><br /><searchLink fieldCode="AR" term="%22Mooley%2C+K%2E+P%2E%22">Mooley, K. P.</searchLink><br /><searchLink fieldCode="AR" term="%22Ravi%2C+V%2E%22">Ravi, V.</searchLink><br /><searchLink fieldCode="AR" term="%22Horesh%2C+A%2E%22">Horesh, A.</searchLink><br /><searchLink fieldCode="AR" term="%22Kasliwal%2C+M%2E+M%2E%22">Kasliwal, M. M.</searchLink><br /><searchLink fieldCode="AR" term="%22Kulkarni%2C+S%2E+R%2E%22">Kulkarni, S. R.</searchLink> – Name: TitleSource Label: Source Group: Src Data: <searchLink fieldCode="JN" term="%22Science+%28pre-March+2025%29%22">Science (pre-March 2025)</searchLink>. 9/3/2021, Vol. 373 Issue 6559, p1125-1129. 5p. 4 Graphs. – Name: Subject Label: Subjects Group: Su Data: <searchLink fieldCode="DE" term="%22Radio+sources+%28Astronomy%29%22">Radio sources (Astronomy)</searchLink><br /><searchLink fieldCode="DE" term="%22Supernovae%22">Supernovae</searchLink><br /><searchLink fieldCode="DE" term="%22Exothermic+reactions%22">Exothermic reactions</searchLink><br /><searchLink fieldCode="DE" term="%22Supergiant+stars%22">Supergiant stars</searchLink><br /><searchLink fieldCode="DE" term="%22Nuclear+fuels%22">Nuclear fuels</searchLink><br /><searchLink fieldCode="DE" term="%22Stellar+mergers%22">Stellar mergers</searchLink><br /><searchLink fieldCode="DE" term="%22Very+large+array+telescopes%22">Very large array telescopes</searchLink><br /><searchLink fieldCode="DE" term="%22Radio+jets+%28Astrophysics%29%22">Radio jets (Astrophysics)</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: A core collapse supernova occurs when exothermic fusion ceases in the core of a massive star, which is typically caused by exhaustion of nuclear fuel. Theory predicts that fusion could be interrupted earlier by merging of the star with a compact binary companion. We report a luminous radio transient, VT J121001+495647, found in the Very Large Array Sky Survey. The radio emission is consistent with supernova ejecta colliding with a dense shell of material, potentially ejected by binary interaction in the centuries before explosion. We associate the supernova with an archival x-ray transient, which implies that a relativistic jet was launched during the explosion. The combination of an early relativistic jet and late-time dense interaction is consistent with expectations for a merger-driven explosion. [ABSTRACT FROM AUTHOR] – Name: AbstractSuppliedCopyright Label: Group: Ab Data: <i>Copyright of Science (pre-March 2025) is the property of American Association for the Advancement of Science 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: 10.1126/science.abg6037 Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 5 StartPage: 1125 Subjects: – SubjectFull: Radio sources (Astronomy) Type: general – SubjectFull: Supernovae Type: general – SubjectFull: Exothermic reactions Type: general – SubjectFull: Supergiant stars Type: general – SubjectFull: Nuclear fuels Type: general – SubjectFull: Stellar mergers Type: general – SubjectFull: Very large array telescopes Type: general – SubjectFull: Radio jets (Astrophysics) Type: general Titles: – TitleFull: A transient radio source consistent with a merger-triggered core collapse supernova. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Dong, D. Z. – PersonEntity: Name: NameFull: Hallinan, G. – PersonEntity: Name: NameFull: Nakar, E. – PersonEntity: Name: NameFull: Ho, A. Y. Q. – PersonEntity: Name: NameFull: Hughes, A. K. – PersonEntity: Name: NameFull: Hotokezaka, K. – PersonEntity: Name: NameFull: Myers, S. T. – PersonEntity: Name: NameFull: De, K. – PersonEntity: Name: NameFull: Mooley, K. P. – PersonEntity: Name: NameFull: Ravi, V. – PersonEntity: Name: NameFull: Horesh, A. – PersonEntity: Name: NameFull: Kasliwal, M. M. – PersonEntity: Name: NameFull: Kulkarni, S. R. IsPartOfRelationships: – BibEntity: Dates: – D: 03 M: 09 Text: 9/3/2021 Type: published Y: 2021 Identifiers: – Type: issn-print Value: 00368075 Numbering: – Type: volume Value: 373 – Type: issue Value: 6559 Titles: – TitleFull: Science (pre-March 2025) Type: main |
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