A mechanism for the superluminal ejections in microquasars: a jet/accretion disk symbiosis (2004)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- Subjects: JATOS (ASTRONOMIA); COSMOLOGIA
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Abstract Book
- Conference titles: Magnetic Fields in the Universe : from Laboratory and Stars to Primordial Structures
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ABNT
GOUVEIA DAL PINO, Elisabete Maria de e LAZARIAN, A. A mechanism for the superluminal ejections in microquasars: a jet/accretion disk symbiosis. 2004, Anais.. s.n.: s.l., 2004. . Acesso em: 24 abr. 2024. -
APA
Gouveia dal Pino, E. M. de, & Lazarian, A. (2004). A mechanism for the superluminal ejections in microquasars: a jet/accretion disk symbiosis. In Abstract Book. s.n.: s.l. -
NLM
Gouveia dal Pino EM de, Lazarian A. A mechanism for the superluminal ejections in microquasars: a jet/accretion disk symbiosis. Abstract Book. 2004 ;[citado 2024 abr. 24 ] -
Vancouver
Gouveia dal Pino EM de, Lazarian A. A mechanism for the superluminal ejections in microquasars: a jet/accretion disk symbiosis. Abstract Book. 2004 ;[citado 2024 abr. 24 ] - 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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