From 3D hydrodynamic simulations of common-envelope interaction to gravitational-wave mergers
Modelling the evolution of progenitors of gravitational-wave merger events in binary stars faces two major uncertainties: the common-envelope phase and supernova kicks. These two processes are critical for the final orbital configuration of double compact-object systems with neutron stars and black...
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| Hauptverfasser: | , , , , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
08 November 2022
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| In: |
Astronomy and astrophysics
Year: 2022, Jahrgang: 667, Pages: 1-16 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/202142731 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: https://doi.org/10.1051/0004-6361/202142731 Verlag, kostenfrei, Volltext: https://www.aanda.org/articles/aa/abs/2022/11/aa42731-21/aa42731-21.html 
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| Verfasserangaben: | Melvin M. Moreno, Fabian R.N. Schneider, Friedrich K. Röpke, Sebastian T. Ohlmann, Rüdiger Pakmor, Philipp Podsiadlowski, and Christian Sand |
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| 245 | 1 | 0 | |a From 3D hydrodynamic simulations of common-envelope interaction to gravitational-wave mergers |c Melvin M. Moreno, Fabian R.N. Schneider, Friedrich K. Röpke, Sebastian T. Ohlmann, Rüdiger Pakmor, Philipp Podsiadlowski, and Christian Sand |
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| 520 | |a Modelling the evolution of progenitors of gravitational-wave merger events in binary stars faces two major uncertainties: the common-envelope phase and supernova kicks. These two processes are critical for the final orbital configuration of double compact-object systems with neutron stars and black holes. Predictive one-dimensional models of common-envelope interaction are lacking and multidimensional simulations are challenged by the vast range of relevant spatial and temporal scales. Here, we present three-dimensional, magnetohydrodynamic simulations of the common-envelope interaction of an initially 10 M⊙ red supergiant primary star with a black-hole and a neutron-star companion. ... | ||
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