3D simulations of strongly magnetized non-rotating supernovae: explosion dynamics and remnant properties

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SEEK ID: https://publications.h-its.org/publications/1756

SEEK ID: https://publications.h-its.org/publications/1756

DOI: 10.1093/mnras/stac3247

Research Groups: Stellar Evolution Theory

Publication type: Journal

Journal: \mnras

Citation: Monthly Notices of the Royal Astronomical Society 518(3):3622-3636

Date Published: 2023

Registered Mode: imported from a bibtex file

Authors: Vishnu Varma, Bernhard Müller, Fabian R. N. Schneider

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Varma, V., Müller, B., & Schneider, F. R. N. (2022). 3D simulations of strongly magnetized non-rotating supernovae: explosion dynamics and remnant properties. In Monthly Notices of the Royal Astronomical Society (Vol. 518, Issue 3, pp. 3622–3636). Oxford University Press (OUP). https://doi.org/10.1093/mnras/stac3247
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Created: 5th Jan 2024 at 16:18

Last updated: 5th Mar 2024 at 21:25

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