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    Subdwarf B stars from the common envelope ejection channel by Xiong, H, Chen, X, Podsiadlowski, P, Han, Z

    Published 2017
    “…One group, referred as the flash-mixing sdBs, almost has no H-rich envelope and crows at the hottest temperature end of the extremely horizontal branch (EHB), while the other group, called as the canonical sdBs, has significant H-rich envelope and spreads over the whole canonical EHB region. …”
    Journal article
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