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arXiv · 2111.13305

Close binary evolution based on Gaia DR2: the origin of late WC-type Wolf-Rayet stars with low luminosity

Weiguo Peng·Hanfeng Song·Georges Meynet·Andre Maeder·Fabio Barblan·Ruiyu Zhang·Sylvia Ekströmt·Cyril Georgy·Gang Long·Liuyan Zhao·Ying Qin
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Abstract

The observed late-type WC Wolf-Rayet stars (WC7-9) with low luminosity below $\rm \log L/L_{\odot} < 5.4$ in the HR diagram cannot be reproduced satisfactorily by the evolutionary track of single stars. The mass transfer due to Roche lobe overflow drastically modifies the internal structure and surface compositions of two components. Therefore, binaries provide a very promising evolutionary channel to produce these WC stars.

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Weiguo Peng, Hanfeng Song, Georges Meynet, Andre Maeder, Fabio Barblan, Ruiyu Zhang, Sylvia Ekströmt, Cyril Georgy, Gang Long, Liuyan Zhao, Ying Qin. 2021-11-26. Close binary evolution based on Gaia DR2: the origin of late WC-type Wolf-Rayet stars with low luminosity. https://doi.org/10.1051/0004-6361%2F202141769

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