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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2 Pith papers cite this work. Polarity classification is still indexing.
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Intermediate-mass mergers explain the disputed origin and B[e] properties of several FS CMa 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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Intermediate-Mass Mergers: A New Scenario for Several FS CMa Stars
Intermediate-mass mergers explain the disputed origin and B[e] properties of several FS CMa stars.