MESA input and results for: A Channel to Form Fast-spinning Black Hole-Neutron Star Binary Mergers as Multimessenger Sources. II. Accretion-induced Spin-up
Authors/Creators
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1.
Guangxi University
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2.
University of Nevada, Las Vegas
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3.
Anhui Normal University
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4.
Monash University
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5.
Qufu Normal University
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6.
Nanchang University
Description
MESA inlists, input files and associated data products for the paper "A Channel to Form Fast-spinning Black Hole-Neutron Star Binary Mergers as Multimessenger Sources. II. Accretion-induced Spin-up". Version 15140 is used.
BH-He stars binary evolution result data are included in ''result.zip'', and folders name match the initial parameters of system, e.g. BHs mass, He-rich stars mass, periods, accretion rates limit. The detailed evolution history is in file ''history.data'', where its initial parameters match the folder name. We evolve He-rich stars until the carbon depletion is reached in the center, we suggest the last line of ''history.data'' is the end of BH-He rich stars evolution course.
BH-NS binary systems evolution sim based on these data with method described in the article.