The mass range of hot subdwarf B stars from MESA simulations
Date Issued
2024-02
Author(s) USM
Piraino-Cerda, F.
DOI
10.1093/mnras/stad3891
Abstract
Hot subdwarf B (sdB) stars are helium core burning stars that have lost almost their entire hydrogen envelope due to binary interaction. Their assumed canonical mass of M-sdB similar to 0.47 M-circle dot has recently been debated given a broad range found
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