Magnetically driven outflows in a starburst environment (1999)
- Authors:
- USP affiliated authors: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG ; TANCO, GUSTAVO ADOLFO MEDINA - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; GALÁXIAS
- Language: Inglês
- Imprenta:
- Source:
- Título: Astrophysical Journal
- Volume/Número/Paginação/Ano: v. 518, n. 1, pt. 1, p. 129-137, June 1999
-
ABNT
GOUVEIA DAL PINO, Elisabete Maria de e MEDINA TANCO, Gustavo Adolfo. Magnetically driven outflows in a starburst environment. Astrophysical Journal, v. 518, n. 1, p. 129-137, 1999Tradução . . Acesso em: 06 nov. 2024. -
APA
Gouveia dal Pino, E. M. de, & Medina Tanco, G. A. (1999). Magnetically driven outflows in a starburst environment. Astrophysical Journal, 518( 1), 129-137. -
NLM
Gouveia dal Pino EM de, Medina Tanco GA. Magnetically driven outflows in a starburst environment. Astrophysical Journal. 1999 ; 518( 1): 129-137.[citado 2024 nov. 06 ] -
Vancouver
Gouveia dal Pino EM de, Medina Tanco GA. Magnetically driven outflows in a starburst environment. Astrophysical Journal. 1999 ; 518( 1): 129-137.[citado 2024 nov. 06 ] - Galactic diffuse 'gama'-ray emission at TeV energies and the ultra-high energy cosmic rays
- Do starbursts have de power to produce jets?
- Evolutive hybrid model for agns: from starbursts to accretion disks in black holes
- Contamination of the cosmic microwave background radiation by diffuse galactic emission
- Photometry of isolated pulsars
- Effects of the local supper-bubble on the cosmic background radiation
- Constraints on the origin of ultra-high energy cosmic rays
- Trajectories of ultra-high energy cosmic rays through the galactic magnetic field
- Non-diffusive propagation of ultra high energy cosmic rays
- Deflection of ultra-high-energy cosmic rays by the galactic magnetic field: from the sources to the detector
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