SPH simulations of clumps formation by dissipative collision of molecular clouds (2000)
Source: Astronomy and Astrophysics Supplement Series. Unidade: IAG
Subjects: ASTRONOMIA, RADIOASTRONOMIA, ASTROFÍSICA ESTELAR, HIDRODINÂMICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
MARINHO, E. P. e LÉPINE, Jacques Raymond Daniel. SPH simulations of clumps formation by dissipative collision of molecular clouds. Astronomy and Astrophysics Supplement Series, v. 142, n. 1, p. 165-179, 2000Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20011352. Acesso em: 10 out. 2024.APA
Marinho, E. P., & Lépine, J. R. D. (2000). SPH simulations of clumps formation by dissipative collision of molecular clouds. Astronomy and Astrophysics Supplement Series, 142( 1), 165-179. doi:10.1051/0004-6361:20011352NLM
Marinho EP, Lépine JRD. SPH simulations of clumps formation by dissipative collision of molecular clouds [Internet]. Astronomy and Astrophysics Supplement Series. 2000 ; 142( 1): 165-179.[citado 2024 out. 10 ] Available from: https://doi.org/10.1051/0004-6361:20011352Vancouver
Marinho EP, Lépine JRD. SPH simulations of clumps formation by dissipative collision of molecular clouds [Internet]. Astronomy and Astrophysics Supplement Series. 2000 ; 142( 1): 165-179.[citado 2024 out. 10 ] Available from: https://doi.org/10.1051/0004-6361:20011352
