Main-sequence companions to massive Be stars
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About 20% of all B-type stars are classical Be stars. The Be phenomenon is strongly correlated with rapid rotation, the origin of which remains unclear. It may be rooted in...
在所有B型恒星（B-type stars）中，约有20%为经典Be星（classical Be stars）。Be现象（Be phenomenon）与快速自转密切相关，但其快速自转的起源仍不明确，其根源可能在于……
