Relativistic MHD simulations of magnetized jets (2013)
- Authors:
- USP affiliated authors: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG ; GONÇALVES, DIEGO ANTONIO FALCETA - EACH
- Unidades: IAG; EACH
- Subjects: RAIOS GAMA; JATOS(ASTRONOMIA)
- Language: Inglês
- Imprenta:
- Publisher: International Astronomical Union
- Publisher place: Paris
- Date published: 2013
- Source:
- Título do periódico: LARIM 2013: Abstract Book
- Conference titles: Latin American Regional IAU Meeting
-
ABNT
ROCHA DA SILVA, G et al. Relativistic MHD simulations of magnetized jets. 2013, Anais.. Paris: International Astronomical Union, 2013. . Acesso em: 27 set. 2024. -
APA
Rocha da Silva, G., Dal Pino, E. M. de G., Falceta-Gonçalves, D., & Kowal, G. (2013). Relativistic MHD simulations of magnetized jets. In LARIM 2013: Abstract Book. Paris: International Astronomical Union. -
NLM
Rocha da Silva G, Dal Pino EM de G, Falceta-Gonçalves D, Kowal G. Relativistic MHD simulations of magnetized jets. LARIM 2013: Abstract Book. 2013 ;[citado 2024 set. 27 ] -
Vancouver
Rocha da Silva G, Dal Pino EM de G, Falceta-Gonçalves D, Kowal G. Relativistic MHD simulations of magnetized jets. LARIM 2013: Abstract Book. 2013 ;[citado 2024 set. 27 ] - Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps
- Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback
- Ambient magnetic field amplification in shock fronts of relativistic jets: an application to GRB afterglows
- Turbulence and dynamo interlinks
- Dynamo in the Intra-Cluster Medium: simulation of CGL-MHD turbulent dynamo
- The ASTRI Mini-Array of cherenkov telescopes at the observatorio del teide
- MHD turbulence-Star Formation Connection: from pc to kpc scales
- Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium
- Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium
- Do dense molecular cores with broad emission spectra at |l| ≈ 5.4○, |b| ≈ 0.4○ trace the Galactic bar? A multi molecular line study from HOPS
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas