Revealing the structure of the outer disks of classical Be stars (2017)
Fonte: The B[e] phenomenon: forty years of studies. Nome do evento: Proceedings of a conference held at Charles University. Unidade: IAG
Assuntos: ASTROFÍSICA ESTELAR, DISCOS DE ACRESÇÃO
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ABNT
KLEMENT, R e CARCIOFI, Alex Cavaliéri e RIVINIUS, T. Revealing the structure of the outer disks of classical Be stars. 2017, Anais.. San Francico: Astronomical Society of the Pacific, 2017. . Acesso em: 30 set. 2024.APA
Klement, R., Carciofi, A. C., & Rivinius, T. (2017). Revealing the structure of the outer disks of classical Be stars. In The B[e] phenomenon: forty years of studies. San Francico: Astronomical Society of the Pacific.NLM
Klement R, Carciofi AC, Rivinius T. Revealing the structure of the outer disks of classical Be stars. The B[e] phenomenon: forty years of studies. 2017 ;[citado 2024 set. 30 ]Vancouver
Klement R, Carciofi AC, Rivinius T. Revealing the structure of the outer disks of classical Be stars. The B[e] phenomenon: forty years of studies. 2017 ;[citado 2024 set. 30 ]
