Prevalence of SED Turndown among Classical Be Stars: Are All Be Stars Close Binaries?

Article (Web of Science)

• cited authors: Klement, Robert; Carciofi, A. C.; Rivinius, T.; Ignace, R.; Matthews, L. D.; Torstensson, K.; Gies, D.; Vieira, R. G.; Richardson, N. D.; de Souza, A. Domiciano; Bjorkman, J. E.; Hallinan, G.; Faes, D. M.; Mota, B.; Gullingsrud, A. D.; de Breuck, C.; Kervella, P.; Cure, M.; Gunawan, D.
• authors: Bjorkman, Jon E
• publication date: November 10, 2019
• webpage: Web of Science
• published in: ASTROPHYSICAL JOURNAL Journal
• category: ASTRONOMY & ASTROPHYSICS Category

keywords

• Be stars
• Binary stars
• Circumstellar disks
• Circumstellar matter
• Early-type emission stars
• Infrared excess
• Radio astronomy
• Radio continuum emission
• Stellar astronomy
• Stellar evolution
• Stellar rotation
• Subdwarf stars

• volume: 885
• issue: 2