Radiation hydrodynamic simulations of massive star formation via gravitationally trapped H II regions: spherically symmetric ionized accretion flows (2019)
- Authors:
- Autor USP: GONÇALVES, DIEGO ANTONIO FALCETA - EACH
- Unidade: EACH
- DOI: 10.1093/mnras/stz621
- Subjects: HIDRODINÂMICA; ASTRONOMIA; ASTROFÍSICA ESTELAR; ESTRELAS; TRANSFERÊNCIA RADIATIVA
- Language: Inglês
- Imprenta:
- Source:
- Título: Royal Astronomical Society. Monthly Notices
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v. 485, p. 3761–3770, Mar. 21019
- Status:
- Artigo possui versão em acesso aberto em repositório (Green Open Access)
- Versão do Documento:
- Versão submetida (Pré-print)
- Acessar versão aberta:
-
ABNT
LUND, K. et al. Radiation hydrodynamic simulations of massive star formation via gravitationally trapped H II regions: spherically symmetric ionized accretion flows. Royal Astronomical Society. Monthly Notices, v. 485, p. 3761–3770, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz621. Acesso em: 07 abr. 2026. -
APA
Lund, K., Wood, K., Gonçalves, D. A. F., Vandenbroucke, B., Sartorio, N. S., Bonnell, I. A., et al. (2019). Radiation hydrodynamic simulations of massive star formation via gravitationally trapped H II regions: spherically symmetric ionized accretion flows. Royal Astronomical Society. Monthly Notices, 485, 3761–3770. doi:10.1093/mnras/stz621 -
NLM
Lund K, Wood K, Gonçalves DAF, Vandenbroucke B, Sartorio NS, Bonnell IA, Johnston KG, Keto E. Radiation hydrodynamic simulations of massive star formation via gravitationally trapped H II regions: spherically symmetric ionized accretion flows [Internet]. Royal Astronomical Society. Monthly Notices. 2019 ; 485 3761–3770.[citado 2026 abr. 07 ] Available from: https://doi.org/10.1093/mnras/stz621 -
Vancouver
Lund K, Wood K, Gonçalves DAF, Vandenbroucke B, Sartorio NS, Bonnell IA, Johnston KG, Keto E. Radiation hydrodynamic simulations of massive star formation via gravitationally trapped H II regions: spherically symmetric ionized accretion flows [Internet]. Royal Astronomical Society. Monthly Notices. 2019 ; 485 3761–3770.[citado 2026 abr. 07 ] Available from: https://doi.org/10.1093/mnras/stz621 - Massive star formation via torus accretion: the effect of photoionization feedback
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