For 14 of 21 observed Wolf-Rayet plus O-star binaries, the authors infer that the first mass-transfer phase began on the main sequence (Case A), with low accretion efficiency and high angular momentum loss.
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WR + O binaries as probes of the first phase of mass transfer
For 14 of 21 observed Wolf-Rayet plus O-star binaries, the authors infer that the first mass-transfer phase began on the main sequence (Case A), with low accretion efficiency and high angular momentum loss.