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ZENODO
Software . 2026
License: CC BY
Data sources: ZENODO
ZENODO
Software . 2026
License: CC BY
Data sources: Datacite
ZENODO
Software . 2026
License: CC BY
Data sources: Datacite
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MESA inlists for The Growth of the Central Black Holes in Quasi-stars (Hassan et al. 2026)

integration_instructionsResearch softwarekeyboard_double_arrow_right Software 20 Jan 2026Publisher:Zenodo
Authors: Hassan, Jake; Perna, Rosalba; Cantiello, Matteo; Armitage, Philip; Begelman, Mitchell; Ryu, Taeho;

doi: 10.5281/zenodo.18319701 , 10.5281/zenodo.18319702

MESA inlists for The Growth of the Central Black Holes in Quasi-stars (Hassan et al. 2026)

Abstract

MESA inlists used for modelling quasi-stars in "The Growth of the Central Black Holes in Quasi-stars" (2026), using both the models from Ball et al. (2011, 2012) and Coughlin & Begelman (2026). These were run using version r24.08.1 of MESA and version 24.7.1 of the MESA SDK. Details on the inlists are described in the README.txt files.

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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