Spectrally and spatially resolved Hα emission from Be stars: their disks rotate Keplerian (2011)
Fonte: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, ESPECTROS, ASTROFÍSICA ESTELAR
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ABNT
OUDMAIJER, René D. et al. Spectrally and spatially resolved Hα emission from Be stars: their disks rotate Keplerian. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311011008. Acesso em: 19 jul. 2024.APA
Oudmaijer, R. D., Wheelwright, H. E., Carciofi, A. C., Bjorkman, J. E., & Bjorkman, K. S. (2011). Spectrally and spatially resolved Hα emission from Be stars: their disks rotate Keplerian. In Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311011008NLM
Oudmaijer RD, Wheelwright HE, Carciofi AC, Bjorkman JE, Bjorkman KS. Spectrally and spatially resolved Hα emission from Be stars: their disks rotate Keplerian [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 jul. 19 ] Available from: https://doi.org/10.1017/S1743921311011008Vancouver
Oudmaijer RD, Wheelwright HE, Carciofi AC, Bjorkman JE, Bjorkman KS. Spectrally and spatially resolved Hα emission from Be stars: their disks rotate Keplerian [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 jul. 19 ] Available from: https://doi.org/10.1017/S1743921311011008
