A magnetic reconnection model for explaining AGNs and microquasars radiation (2013)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- Subjects: QUASARES; DISCOS DE ACRESÇÃO; RAIOS CÓSMICOS; MAGNETISMO
- 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
KHIALI, B et al. A magnetic reconnection model for explaining AGNs and microquasars radiation. 2013, Anais.. Paris: International Astronomical Union, 2013. . Acesso em: 14 maio 2024. -
APA
Khiali, B., Dal Pino, E. M. de G., Del Valle, M. V., Kowal, G., & Sol, H. (2013). A magnetic reconnection model for explaining AGNs and microquasars radiation. In LARIM 2013: Abstract Book. Paris: International Astronomical Union. -
NLM
Khiali B, Dal Pino EM de G, Del Valle MV, Kowal G, Sol H. A magnetic reconnection model for explaining AGNs and microquasars radiation. LARIM 2013: Abstract Book. 2013 ;[citado 2024 maio 14 ] -
Vancouver
Khiali B, Dal Pino EM de G, Del Valle MV, Kowal G, Sol H. A magnetic reconnection model for explaining AGNs and microquasars radiation. LARIM 2013: Abstract Book. 2013 ;[citado 2024 maio 14 ] - 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
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