Journal article Open Access

# Testing models of accreting stars in massive binaries on ζ Ophiuchi

Renzo, Mathieu; Gotberg, Ylva

Input and output files for MESA r15140 described in [Renzo & Gotberg 2021](https://ui.adsabs.harvard.edu/abs/2021arXiv210710933R/abstract).

fiducial.tar.xz contains the MESA work directories and output for the evolution of the model described in Sec. 3, one for the evolution in a binary, and one after detachment to finish the main sequence of the accreting star.

single_stars.tar.xz contains rotating single star models labeled according to their initial mass, and for each mass non-rotating (no-rot) and rotating models (labelled based on the initial omega/omega_crit) are provided.

The other tarballs contain structures similar to best_model.tar.gz with parameter variations (see Sec. 6 and README.org).

All parameter variations described in the paper can be obtained by modifying one (or more) parameters from the input files contained in these folders.

A git repository for this project is available at https://github.com/mathren90/zeta_oph

Files (14.3 GB)
Name Size
Brott+11_ov.tar.xz
md5:8b37fa159e25fccc0b95c972651a9ed9
273.4 MB
composition_accretor.mp4
md5:f27c564825c0c1e4b04668f8b00f2ff7
5.2 MB
do_J_accretion.tar.xz
md5:660f2bfaba7907221c690a02d02f4572
142.8 MB
ES_10x_lower.tar.xz
md5:c612da7771fc729eda282997c62e15ce
275.1 MB
fiducial.tar.xz
md5:c5e670bda72c4dfdb0bc468b3d41cb75
11.4 GB
M1_25_M2_17_P75_Z0.01.tar.xz
md5:f3f3d3ab59e926ef29c04670369fd6b8
195.2 MB
M1_30.tar.xz
md5:f6914e6e7736a5fe686aa9e2cef108cf
224.6 MB
mix_movie.mp4
md5:479c7a9e4ca6c60262ca1098123af75c
2.7 MB
period75days.tar.xz
md5:e01929db88e1a405acaaf091ac3d45a3
336.0 MB
md5:5deacddde09f7d32459b827ae31bf2b9
2.0 kB
single_stars.tar.xz
768.0 MB
space_res.tar.xz
md5:003af696167757d7208c4b0eacaf309b
332.3 MB
Z_0.0142.tar.xz
md5:bd448a31639ab06cbb0ba3cd91013302
412.4 MB
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