Intermediate-mass mergers explain the disputed origin and B[e] properties of several FS CMa stars.
Tracing Physical Processes Affecting Spectral Formation in the Low-luminosity B[e] Stars of the FS CMa Group
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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.