Binary-stripped Stars as Core-collapse Supernovae Progenitors
Abstract
Most massive stars experience binary interactions in their lifetimes that can alter both the surface and core structure of the stripped star with significant effects on their ultimate fate as core-collapse supernovae. However, core-collapse supernovae simulations to date have focused almost exclusively on the evolution of single stars. We present a systematic simulation study of single and binary-stripped stars with the same initial mass as candidates for core-collapse supernovae (11–21 M⊙). Generally, we find that binary-stripped stars core tend to have a smaller compactness parameter, with a more prominent, deeper silicon/oxygen interface, and explode preferentially to the corresponding single stars of the same initial mass. Such a dichotomy of behavior between these two modes of evolution would have important implications for supernovae statistics, including the final neutron star masses, explosion energies, and nucleosynthetic yields. Binary-stripped remnants are also well poised to populate the possible mass gap between the heaviest neutron stars and the lightest black holes. Our work presents an improvement along two fronts, as we self-consistently account for the pre-collapse stellar evolution and the subsequent explosion outcome. Even so, our results emphasize the need for more detailed stellar evolutionary models to capture the sensitive nature of explosion outcome.
- Authors:
-
[1];
[2];
[3];
[4];
[5];
[6]
- Univ. of California, Berkeley, CA (United States). Department of Physics and Astronomy
- Univ. of Amsterdam (Netherlands). Anton Pannekoek Institute of Astronomy and GRAPPA
- Columbia Univ., New York, NY (United States). Department of Physics; Flatiron Institute, New York, NY (United States). Center for Computational Astrophysics
- The Observatories of the Carnegie Institution for Science, Pasadena, CA (United States)
- Princeton Univ., NJ (United States). Department of Astrophysical Sciences
- Univ. of Amsterdam (Netherlands). Anton Pannekoek Institute of Astronomy and GRAPPA; Max Planck Institute for Astrophysics, Garching (Germany); Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Publication Date:
- Research Org.:
- Univ. of California, Oakland, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1852582
- Grant/Contract Number:
- SC0018297
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal. Letters
- Additional Journal Information:
- Journal Volume: 916; Journal Issue: 1; Journal ID: ISSN 2041-8205
- Publisher:
- IOP Publishing
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics
Citation Formats
Vartanyan, David, Laplace, Eva, Renzo, Mathieu, Götberg, Ylva, Burrows, Adam, and de Mink, Selma E. Binary-stripped Stars as Core-collapse Supernovae Progenitors. United States: N. p., 2021.
Web. doi:10.3847/2041-8213/ac0b42.
Vartanyan, David, Laplace, Eva, Renzo, Mathieu, Götberg, Ylva, Burrows, Adam, & de Mink, Selma E. Binary-stripped Stars as Core-collapse Supernovae Progenitors. United States. https://doi.org/10.3847/2041-8213/ac0b42
Vartanyan, David, Laplace, Eva, Renzo, Mathieu, Götberg, Ylva, Burrows, Adam, and de Mink, Selma E. Fri .
"Binary-stripped Stars as Core-collapse Supernovae Progenitors". United States. https://doi.org/10.3847/2041-8213/ac0b42. https://www.osti.gov/servlets/purl/1852582.
@article{osti_1852582,
title = {Binary-stripped Stars as Core-collapse Supernovae Progenitors},
author = {Vartanyan, David and Laplace, Eva and Renzo, Mathieu and Götberg, Ylva and Burrows, Adam and de Mink, Selma E.},
abstractNote = {Most massive stars experience binary interactions in their lifetimes that can alter both the surface and core structure of the stripped star with significant effects on their ultimate fate as core-collapse supernovae. However, core-collapse supernovae simulations to date have focused almost exclusively on the evolution of single stars. We present a systematic simulation study of single and binary-stripped stars with the same initial mass as candidates for core-collapse supernovae (11–21 M⊙). Generally, we find that binary-stripped stars core tend to have a smaller compactness parameter, with a more prominent, deeper silicon/oxygen interface, and explode preferentially to the corresponding single stars of the same initial mass. Such a dichotomy of behavior between these two modes of evolution would have important implications for supernovae statistics, including the final neutron star masses, explosion energies, and nucleosynthetic yields. Binary-stripped remnants are also well poised to populate the possible mass gap between the heaviest neutron stars and the lightest black holes. Our work presents an improvement along two fronts, as we self-consistently account for the pre-collapse stellar evolution and the subsequent explosion outcome. Even so, our results emphasize the need for more detailed stellar evolutionary models to capture the sensitive nature of explosion outcome.},
doi = {10.3847/2041-8213/ac0b42},
journal = {The Astrophysical Journal. Letters},
number = 1,
volume = 916,
place = {United States},
year = {Fri Jul 23 00:00:00 EDT 2021},
month = {Fri Jul 23 00:00:00 EDT 2021}
}
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