Single Be stars form as ejected companions from Type Ia supernovae in about 0.4% of helium star plus main-sequence star binaries, with 22% becoming runaway stars.
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Magnetic fields in Be stars reach up to 460 G, much stronger than the under-100 G values reported in earlier studies, based on new spectropolarimetric observations of seven stars.
citing papers explorer
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A New Pathway to Single Be Stars: Ejected Companions from Type Ia Supernovae
Single Be stars form as ejected companions from Type Ia supernovae in about 0.4% of helium star plus main-sequence star binaries, with 22% becoming runaway stars.
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The magnetic fields in Be stars are stronger than previously suggested
Magnetic fields in Be stars reach up to 460 G, much stronger than the under-100 G values reported in earlier studies, based on new spectropolarimetric observations of seven stars.