MHD numerical simulations of Perseus A: formation of filaments and magnetic loops (2009)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- Subjects: GALÁXIAS; AGLOMERADOS DE GALÁXIAS; MÉTODOS NUMÉRICOS
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Cosmic magnetic fields: from planets, to stars and galaxies
- Conference titles: IAU Symposium
-
ABNT
GONÇALVES, Diego Falceta e DAL PINO, Elisabete Maria de Gouveia e GALLAGHER III, J. MHD numerical simulations of Perseus A: formation of filaments and magnetic loops. 2009, Anais.. Paris: IAU, 2009. . Acesso em: 03 maio 2024. -
APA
Gonçalves, D. F., Dal Pino, E. M. de G., & Gallagher III, J. (2009). MHD numerical simulations of Perseus A: formation of filaments and magnetic loops. In Cosmic magnetic fields: from planets, to stars and galaxies. Paris: IAU. -
NLM
Gonçalves DF, Dal Pino EM de G, Gallagher III J. MHD numerical simulations of Perseus A: formation of filaments and magnetic loops. Cosmic magnetic fields: from planets, to stars and galaxies. 2009 ;[citado 2024 maio 03 ] -
Vancouver
Gonçalves DF, Dal Pino EM de G, Gallagher III J. MHD numerical simulations of Perseus A: formation of filaments and magnetic loops. Cosmic magnetic fields: from planets, to stars and galaxies. 2009 ;[citado 2024 maio 03 ] - The effects of magnetic fields on radiative cooling jets
- Origin of the superluminal ejections in microquasars by violent magnetic reconnection
- Star formation in 'beta' pictoris triggered by a supernova
- Astrophysical jets and outflows
- Plasmas e altas energias
- Three-dimensional numerical simulations of rotating jets
- Numerical simulations of young stellar jets: from one tenth to parsec scales
- Cosmic magnetic fields: from stars to the primordial universe
- Probing magneto-centrifugal scenarios for jet production
- On the production and acceleration of astrophysical jets: a comparative study
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
