An empirical pipeline for determining the viscosity parameter for Be star disks (2015)
Source: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307. Conference titles: IAU Symposium. Unidade: IAG
Subjects: HIDRODINÂMICA, TRANSFERÊNCIA RADIATIVA, FOTOMETRIA, ESTRELAS, PERDA DE MASSA
ABNT
RÍMULO, Leandro R et al. An empirical pipeline for determining the viscosity parameter for Be star disks. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921314006541. Acesso em: 25 jun. 2024.APA
Rímulo, L. R., Carciofi, A. C., Rivinius, T., & Haubois, X. (2015). An empirical pipeline for determining the viscosity parameter for Be star disks. In New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307. Paris: International Astronomical Union. doi:10.1017/S1743921314006541NLM
Rímulo LR, Carciofi AC, Rivinius T, Haubois X. An empirical pipeline for determining the viscosity parameter for Be star disks [Internet]. New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307. 2015 ;[citado 2024 jun. 25 ] Available from: https://doi.org/10.1017/S1743921314006541Vancouver
Rímulo LR, Carciofi AC, Rivinius T, Haubois X. An empirical pipeline for determining the viscosity parameter for Be star disks [Internet]. New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307. 2015 ;[citado 2024 jun. 25 ] Available from: https://doi.org/10.1017/S1743921314006541