Source: Royal Astronomical Society. Monthly Notices. Unidade: EACH
Subjects: HIDRODINÂMICA, ASTRONOMIA, ASTROFÍSICA ESTELAR, ESTRELAS, TRANSFERÊNCIA RADIATIVA
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: 16 maio 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 maio 16 ] 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 maio 16 ] Available from: https://doi.org/10.1093/mnras/stz621