The Variable Line Width of Achernar (2016)
Fonte: Bright emissaries: Be stars as messengers of star-disk physics :|bproceedings of a meeting held at the University of Western Ontario, in London, Ontario, Canada, on 11-13 August 2014. Unidade: IAG
Assunto: ASTROFÍSICA ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
RIVINIUS, Th. et al. The Variable Line Width of Achernar. 2016, Anais.. San Francisco: Astronomical Society of the Pacific, 2016. Disponível em: https://arxiv.org/pdf/1602.03452.pdf. Acesso em: 30 jun. 2024.APA
Rivinius, T., Townsend, R. H. D., Carciofi, A. C., Leister, N. V., & Stefl, S. (2016). The Variable Line Width of Achernar. In Bright emissaries: Be stars as messengers of star-disk physics :|bproceedings of a meeting held at the University of Western Ontario, in London, Ontario, Canada, on 11-13 August 2014. San Francisco: Astronomical Society of the Pacific. Recuperado de https://arxiv.org/pdf/1602.03452.pdfNLM
Rivinius T, Townsend RHD, Carciofi AC, Leister NV, Stefl S. The Variable Line Width of Achernar [Internet]. Bright emissaries: Be stars as messengers of star-disk physics :|bproceedings of a meeting held at the University of Western Ontario, in London, Ontario, Canada, on 11-13 August 2014. 2016 ;[citado 2024 jun. 30 ] Available from: https://arxiv.org/pdf/1602.03452.pdfVancouver
Rivinius T, Townsend RHD, Carciofi AC, Leister NV, Stefl S. The Variable Line Width of Achernar [Internet]. Bright emissaries: Be stars as messengers of star-disk physics :|bproceedings of a meeting held at the University of Western Ontario, in London, Ontario, Canada, on 11-13 August 2014. 2016 ;[citado 2024 jun. 30 ] Available from: https://arxiv.org/pdf/1602.03452.pdf
