Be discs in coplanar circular binaries: Phase-locked variations of emission lines (2018)
Fonte: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG
Assuntos: HIDRODINÂMICA, ESTRELAS BINÁRIAS
ABNT
PANOGLOU, Despina et al. Be discs in coplanar circular binaries: Phase-locked variations of emission lines. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v. 473, p. 3039-3050, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx2497. Acesso em: 25 out. 2024.APA
Panoglou, D., Faes, D. M., Carciofi, A. C., Okazaki, A. T., Baade, D., Rivinius, T., & Fernandes, M. B. (2018). Be discs in coplanar circular binaries: Phase-locked variations of emission lines. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 473, 3039-3050. doi:10.1093/mnras/stx2497NLM
Panoglou D, Faes DM, Carciofi AC, Okazaki AT, Baade D, Rivinius T, Fernandes MB. Be discs in coplanar circular binaries: Phase-locked variations of emission lines [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2018 ;473 3039-3050.[citado 2024 out. 25 ] Available from: https://doi.org/10.1093/mnras/stx2497Vancouver
Panoglou D, Faes DM, Carciofi AC, Okazaki AT, Baade D, Rivinius T, Fernandes MB. Be discs in coplanar circular binaries: Phase-locked variations of emission lines [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2018 ;473 3039-3050.[citado 2024 out. 25 ] Available from: https://doi.org/10.1093/mnras/stx2497