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ZENODO
Model . 2024
License: CC BY
Data sources: ZENODO
ZENODO
Model . 2024
License: CC BY
Data sources: Datacite
ZENODO
Model . 2024
License: CC BY
Data sources: Datacite
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Evolution of binaries containing a hot subdwarf and a white dwarf to double white dwarfs, and double detonation supernovae with hypervelocity runaway stars

Authors: Rajamuthukumar, Abinaya Swaruba; Bauer, Evan; Pakmor, Ruediger; Justham, Stephen;

Evolution of binaries containing a hot subdwarf and a white dwarf to double white dwarfs, and double detonation supernovae with hypervelocity runaway stars

Abstract

MESA inlists and other input files used for the paper "Evolution of Binaries Containing a Hot Subdwarf and a White Dwarf to Double White Dwarfs and Double Detonation Supernovae with Hypervelocity Runaway Stars." These files were generated using a modified MESA version r23.05.1. A modification was made to the binary_mdot.f90 file to alter the composition of the accretion stream, converting the mass fraction of H to He throughout accretion. This adjustment was implemented to reduce computational time associated with modeling H novae, as the study focuses on He novae and supernovae. For further details, please refer to Section 2 of the paper. The modified binary_mdot.f90 file is also included in this repository.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average