SPH simulations of clumps formation by dissipative collision of molecular clouds

SPH simulations of clumps formation by dissipative collision of molecular clouds (2000)

Authors:
- Marinho, E. P. - Universidade Estadual Paulista Júlio de Mesquita Filho (UNESP)
- Lépine, Jacques Raymond Daniel
Autor USP: LEPINE, JACQUES RAYMOND DANIEL - IAG
Unidade: IAG
DOI: 10.1051/0004-6361:20011352
Subjects: ASTRONOMIA; RADIOASTRONOMIA; ASTROFÍSICA ESTELAR; HIDRODINÂMICA
Language: Inglês
Imprenta:
- Publisher place: Les Ulis
- Date published: 2000
Source:
- Título: Astronomy and Astrophysics Supplement Series
- ISSN: 0365-0138
- Volume/Número/Paginação/Ano: v. 142, n. 1, p. 165-179, Feb. 2000

Informações sobre o DOI: 10.1051/0004-6361:20011352 (Fonte: oaDOI API)

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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: 23 jan. 2026.
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:10.1051/0004-6361:20011352
NLM

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 2026 jan. 23 ] Available from: https://doi.org/10.1051/0004-6361:20011352
Vancouver

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 2026 jan. 23 ] Available from: https://doi.org/10.1051/0004-6361:20011352