Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor (2015)
- Authors:
- Autor USP: GONÇALVES, DIEGO ANTONIO FALCETA - EACH
- Unidade: EACH
- DOI: 10.1088/0004-637X/805/2/109
- Subjects: GALÁXIAS; EVOLUÇÃO ESTELAR; HIDRODINÂMICA
- Language: Inglês
- Imprenta:
- Publisher place: Philadelphia
- Date published: 2015
- Source:
- Título: The Astrophysical Journal
- ISSN: 0004-637X
- Volume/Número/Paginação/Ano: v. 805, n. 2, p. 1-12, jun. 2015
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
-
ABNT
CAPRONI, Anderson et al. Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor. The Astrophysical Journal, v. 805, n. ju 2015, p. 1-12, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/805/2/109. Acesso em: 28 dez. 2025. -
APA
Caproni, A., Lanfranchi, G. A., Silva, A. L. da, & Gonçalves, D. A. F. (2015). Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor. The Astrophysical Journal, 805( ju 2015), 1-12. doi:10.1088/0004-637X/805/2/109 -
NLM
Caproni A, Lanfranchi GA, Silva AL da, Gonçalves DAF. Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor [Internet]. The Astrophysical Journal. 2015 ; 805( ju 2015): 1-12.[citado 2025 dez. 28 ] Available from: https://doi.org/10.1088/0004-637X/805/2/109 -
Vancouver
Caproni A, Lanfranchi GA, Silva AL da, Gonçalves DAF. Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor [Internet]. The Astrophysical Journal. 2015 ; 805( ju 2015): 1-12.[citado 2025 dez. 28 ] Available from: https://doi.org/10.1088/0004-637X/805/2/109 - Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium
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Informações sobre o DOI: 10.1088/0004-637X/805/2/109 (Fonte: oaDOI API)
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