Galactic outflows from PC to KPC scales (2012)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- Subjects: GALÁXIAS; SUPERNOVAS; GÁS INTERESTELAR
- Language: Inglês
- Imprenta:
- Publisher: Sociedade Astronômica Brasileira
- Publisher place: São Paulo
- Date published: 2012
- Conference titles: Reunião Anual da Sociedade Astronômica Brasileira
-
ABNT
MELIOLI, Claudio et al. Galactic outflows from PC to KPC scales. 2012, Anais.. São Paulo: Sociedade Astronômica Brasileira, 2012. . Acesso em: 10 jan. 2026. -
APA
Melioli, C., Dal Pino, E. M. de G., Brighenti, F., D'Ercole, A., & Geraissate, F. (2012). Galactic outflows from PC to KPC scales. In . São Paulo: Sociedade Astronômica Brasileira. -
NLM
Melioli C, Dal Pino EM de G, Brighenti F, D'Ercole A, Geraissate F. Galactic outflows from PC to KPC scales. 2012 ;[citado 2026 jan. 10 ] -
Vancouver
Melioli C, Dal Pino EM de G, Brighenti F, D'Ercole A, Geraissate F. Galactic outflows from PC to KPC scales. 2012 ;[citado 2026 jan. 10 ] - 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
- 3D hydrodynamical simulations of galactic winds: an application to the starburst galaxy M82
- 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
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
