The mass-loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts (2013)
- Authors:
- USP affiliated authors: GONÇALVES, DIEGO ANTONIO FALCETA - EACH
- Unidades: EACH
- DOI: 10.1093/mnras/sts425
- Subjects: GALÁXIAS; ESTRELAS; MATÉRIA ESCURA; EVOLUÇÃO ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Monthly Notices of the Royal Astronomical Society
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v. 429, n. 2, p. 1437\20131449, feb. 2013
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
ABNT
RUIZ, L. O; FALCETA GONÇALVES, Diego Antonio; LANFRANCHI, Gustavo Amaral; CAPRONI, Anderson. The mass-loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts. Monthly Notices of the Royal Astronomical Society, Oxford, v. 429, n. 2, p. 1437\20131449, 2013. Disponível em: < http://dx.doi.org/10.1093/mnras/sts425 > DOI: 10.1093/mnras/sts425. -
APA
Ruiz, L. O., Falceta Gonçalves, D. A., Lanfranchi, G. A., & Caproni, A. (2013). The mass-loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts. Monthly Notices of the Royal Astronomical Society, 429( 2), 1437\20131449. doi:10.1093/mnras/sts425 -
NLM
Ruiz LO, Falceta Gonçalves DA, Lanfranchi GA, Caproni A. The mass-loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 429( 2): 1437\20131449.Available from: http://dx.doi.org/10.1093/mnras/sts425 -
Vancouver
Ruiz LO, Falceta Gonçalves DA, Lanfranchi GA, Caproni A. The mass-loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 429( 2): 1437\20131449.Available from: http://dx.doi.org/10.1093/mnras/sts425 - Radiation hydrodynamic simulations of massive star formation via gravitationally trapped H II regions: spherically symmetric ionized accretion flows
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Informações sobre o DOI: 10.1093/mnras/sts425 (Fonte: oaDOI API)
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