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Dettagli Bibliografici
Autori principali: Korcakova, Daniela, Dvorakova, Nela, Lozano, Iris Bermejo, Wade, Gregg A., Basurto, Alicia Moranchel, Kroupa, Pavel, Chametla, Raul Ortega, Folsom, Colin Peter, Juhas, Ondrej
Natura: Preprint
Pubblicazione: 2026
Soggetti:
Accesso online:https://arxiv.org/abs/2604.11907
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Sommario:
  • We summarise the properties and nature of a peculiar group of B-type stars called FS CMa stars. These stars show the B[e] phenomenon, i.e., their spectra exhibit both forbidden emission lines and infrared excess. Such properties point to an extended circumstellar gas and dust component. Although the phenomenon has been explained in most B[e] stars, the origin and nature of FS CMa stars is disputed. Here, we focus on the merger hypothesis, for which evidence has recently been discovered.