Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations (2013)
- Authors:
- USP affiliated author: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- School: IAG
- DOI: 10.1093/mnras/stt126
- Subjects: MEIO INTERESTELAR; ABUNDÂNCIAS (ASTRONOMIA); JATOS (ASTRONOMIA); GALÁXIAS
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Monthly Notices of the Royal Astronomical Society
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v. 430, p. 3235-3248, 2013
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
ABNT
MELIOLI, C e DAL PINO, Elisabete Maria de Gouveia e GERAISSATE, F. G. Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations. Monthly Notices of the Royal Astronomical Society, v. 430, p. 3235-3248, 2013Tradução . . Disponível em: http://dx.doi.org/10.1093/mnras/stt126. Acesso em: 30 jun. 2022. -
APA
Melioli, C., Dal Pino, E. M. de G., & Geraissate, F. G. (2013). Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations. Monthly Notices of the Royal Astronomical Society, 430, 3235-3248. doi:10.1093/mnras/stt126 -
NLM
Melioli C, Dal Pino EM de G, Geraissate FG. Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 430 3235-3248.[citado 2022 jun. 30 ] Available from: http://dx.doi.org/10.1093/mnras/stt126 -
Vancouver
Melioli C, Dal Pino EM de G, Geraissate FG. Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 430 3235-3248.[citado 2022 jun. 30 ] Available from: http://dx.doi.org/10.1093/mnras/stt126 - Jet-ISM cloud interactions: 3D simulations of the HH 270/110 jet system
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- Exploring a different geometry for the solar tachocline in kinematic solar dynamo model
- On the production and acceleration of astrophysical jets: a comparative study
- Turbulent magnetic reconnection as a possible solution for the magnetic braking problem in protostellar disks
- Numerical study of turbulence of the intracluster medium using a collisionless MHD model
Informações sobre o DOI: 10.1093/mnras/stt126 (Fonte: oaDOI API)
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