Asteroseismic data show sdB stars rotate faster than expected, suggesting transient accretion from common-envelope remnants spins them up via magnetic fields.
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Multi-survey analysis of 157 hot subdwarf binaries yields 23 orbital solutions (11 new) whose mass-period distribution matches post-common-envelope systems, supporting a common-envelope origin.
citing papers explorer
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Asteroseismic rotation rates of hot subdwarf B stars hint at transient accretion from leftover common envelope matter
Asteroseismic data show sdB stars rotate faster than expected, suggesting transient accretion from common-envelope remnants spins them up via magnetic fields.
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Characterizing Orbital Parameters of Hot Subdwarf Binaries with Multiple Spectroscopic Surveys
Multi-survey analysis of 157 hot subdwarf binaries yields 23 orbital solutions (11 new) whose mass-period distribution matches post-common-envelope systems, supporting a common-envelope origin.