Fonte: Royal Astronomical Society. Monthly Notices. Unidade: EACH
Assuntos: HIDRODINÂMICA, ASTRONOMIA, ASTROFÍSICA ESTELAR, ESTRELAS, TRANSFERÊNCIA RADIATIVA
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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: 19 abr. 2024.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/stz621NLM
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 2024 abr. 19 ] Available from: https://doi.org/10.1093/mnras/stz621Vancouver
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 2024 abr. 19 ] Available from: https://doi.org/10.1093/mnras/stz621
