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Filtros : "HIDRODINÂMICA" "IAU Symposium" Removidos: "Rodrigues, Wendel Johnson" "ATAKE, IGOR RUIZ" Limpar

Filtros

Trabalho de evento
Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations (2015)
Melioli, Claudio; Dal Pino, Elisabete Maria de Gouveia
Source: Proceedings IAU Symposium, 313: Extragalactic jets from every angle. Conference titles: IAU Symposium. Unidade: IAG
Subjects: GALÁXIAS SEY FERT, JATOS (ASTRONOMIA), HIDRODINÂMICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
MELIOLI, Claudio e DAL PINO, Elisabete Maria de Gouveia. Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921315002550. Acesso em: 10 out. 2024.
APA
Melioli, C., & Dal Pino, E. M. de G. (2015). Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations. In Proceedings IAU Symposium, 313: Extragalactic jets from every angle. Paris: International Astronomical Union. doi:10.1017/S1743921315002550
NLM
Melioli C, Dal Pino EM de G. Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations [Internet]. Proceedings IAU Symposium, 313: Extragalactic jets from every angle. 2015 ;[citado 2024 out. 10 ] Available from: https://doi.org/10.1017/S1743921315002550
Vancouver
Melioli C, Dal Pino EM de G. Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations [Internet]. Proceedings IAU Symposium, 313: Extragalactic jets from every angle. 2015 ;[citado 2024 out. 10 ] Available from: https://doi.org/10.1017/S1743921315002550
Trabalho de evento
An empirical pipeline for determining the viscosity parameter for Be star disks (2015)
Rímulo, Leandro R; Carciofi, Alex Cavaliéri; Rivinius, Thomas; Haubois, Xavier
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 10 out. 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/S1743921314006541
NLM
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 out. 10 ] Available from: https://doi.org/10.1017/S1743921314006541
Vancouver
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 out. 10 ] Available from: https://doi.org/10.1017/S1743921314006541

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