3D hydrodynamical simulations of galactic winds: an application to the starburst galaxy M82 (2011)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- Subjects: ASTROFÍSICA ESTELAR; GALÁXIAS
- Language: Inglês
- Imprenta:
- Source:
- Conference titles: Reunião Anual da Sociedade Astronômica Brasileira
-
ABNT
GERAISSATE, Fernanda e DAL PINO, Elisabete Maria de Gouveia e MELIOLI, Claudio. 3D hydrodynamical simulations of galactic winds: an application to the starburst galaxy M82. 2011, Anais.. São Paulo: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, 2011. Disponível em: http://www.sab-astro.org.br/sab36/LIVRO.pdf. Acesso em: 10 jan. 2026. -
APA
Geraissate, F., Dal Pino, E. M. de G., & Melioli, C. (2011). 3D hydrodynamical simulations of galactic winds: an application to the starburst galaxy M82. In Resumos. São Paulo: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. Recuperado de http://www.sab-astro.org.br/sab36/LIVRO.pdf -
NLM
Geraissate F, Dal Pino EM de G, Melioli C. 3D hydrodynamical simulations of galactic winds: an application to the starburst galaxy M82 [Internet]. Resumos. 2011 ;[citado 2026 jan. 10 ] Available from: http://www.sab-astro.org.br/sab36/LIVRO.pdf -
Vancouver
Geraissate F, Dal Pino EM de G, Melioli C. 3D hydrodynamical simulations of galactic winds: an application to the starburst galaxy M82 [Internet]. Resumos. 2011 ;[citado 2026 jan. 10 ] Available from: http://www.sab-astro.org.br/sab36/LIVRO.pdf - Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection
- Prospect on intergalactic magnetic field measurements with gamma-ray instruments
- A magnetic reconnection model for explaining the multiwave length emission of the microquasars Cyg X-1 and Cyg X-3
- Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not?
- Multiwavelength temporal and spectral variability of the blazar OJ 287 during and after the 2015 December flare: a major accretion disc contribution
- The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays
- Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs
- Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations
- Gamma-ray flux distribution and nonlinear behavior of four lat bright AGNs
- The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas