Prevalence of SED Turndown among Classical Be Stars: Are All Be Stars Close Binaries? Article (Web of Science)

International Collaboration

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.

publication date

  • November 10, 2019

webpage

published in

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