VizieR Online Data Catalog: Binary mass transfer model data (Schneider+, 2024)

The stellar models were computed with revision 10398 of the Modules-for-Experiments-in-Stellar-Astrophysics (MESA) software package (Paxton et al., 2011ApJS..192....3P, 2013ApJS..208....4P, 2015ApJS..220...15P, 2018ApJS..234...34P, 2019ApJS..243...10P). We used the same basic MESA setup as in Schneider et al. (2021A&A...645A...5S) and briefly summarise it in Sect. 2.1. In Sect. 2.2, we explain how we model binary-star accretion. For comparison of these accretion models with genuine single stars, we employ the single-star models of Schneider et al. (2021A&A...645A...5S). In Sect. 2.3, we briefly describe how we coupled our models to a SN code to study their final fates and possible SN explosions. An overview of all models and key properties discussed in this work are provided in Table A.1. MESA inlists and other settings required to reproduce our models are published online on Zenodo (https://zenodo.org/doi/10.5281/zenodo.10731998).

(1 data file).