Classical Be Stars and Classical Be Star Binaries from LAMOST DR12
Classical Be (CBe) stars are rapidly rotating B-type stars with Balmer emission lines that originate from the decretion disks surrounding them in their spectra. Accounting for ∼20% of all B-type stars, most CBe stars are thought to form through mass and angular momentum transfer from their companion...
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| Principais autores: | , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
IOP Publishing
2026-01-01
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| Colecção: | The Astrophysical Journal Supplement Series |
| Assuntos: | |
| Acesso em linha: | https://doi.org/10.3847/1538-4365/ae450d |
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