The interaction of core-collapse supernova ejecta with a companion star
The progenitors of many core-collapse supernovae (CCSNe) are expected to be in binary systems. After the SN explosion in a binary, the companion star may suffer from mass stripping and be shock heated as a result of the impact of the SN ejecta. If the binary system is disrupted by the SN explosion,...
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| Hauptverfasser: | , , , , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
13 November 2015
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| In: |
Astronomy and astrophysics
Year: 2015, Jahrgang: 584 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/201526757 |
| Online-Zugang: | Resolving-System, lizenzpflichtig, Volltext: https://doi.org/10.1051/0004-6361/201526757 Verlag, lizenzpflichtig, Volltext: https://www.aanda.org/articles/aa/abs/2015/12/aa26757-15/aa26757-15.html 
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| Verfasserangaben: | Zheng-Wei Liu, T.M. Tauris, F.K. Röpke, T.J. Moriya, M. Kruckow, R.J. Stancliffe, and R.G. Izzard |
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| 520 | |a The progenitors of many core-collapse supernovae (CCSNe) are expected to be in binary systems. After the SN explosion in a binary, the companion star may suffer from mass stripping and be shock heated as a result of the impact of the SN ejecta. If the binary system is disrupted by the SN explosion, the companion star is ejected as a runaway star, and in some cases as a hypervelocity star. By performing a series of three-dimensional (3D) hydrodynamical simulations of the collision of SN ejecta with the companion star, we investigate how CCSN explosions affect their binary companion. | ||
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| 700 | 1 | |a Kruckow, M. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Stancliffe, R. J. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Izzard, R. G. |e VerfasserIn |4 aut | |
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