Precession of the Giant HH 34 outflow: a possible jet deceleration mechanism (2002)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- Assunto: ASTRONOMIA
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Astrophysical Journal
- ISSN: 0004-637X
- Volume/Número/Paginação/Ano: v. 580, p. 950-958, 2002
-
ABNT
MASCIADRI, E; GOUVEIA DAL PINO, Elisabete Maria de; RAGA, A C; NORIEGA-CRESPO, A. Precession of the Giant HH 34 outflow: a possible jet deceleration mechanism. Astrophysical Journal, Chicago, v. 580, p. 950-958, 2002. -
APA
Masciadri, E., Gouveia dal Pino, E. M. de, Raga, A. C., & Noriega-Crespo, A. (2002). Precession of the Giant HH 34 outflow: a possible jet deceleration mechanism. Astrophysical Journal, 580, 950-958. -
NLM
Masciadri E, Gouveia dal Pino EM de, Raga AC, Noriega-Crespo A. Precession of the Giant HH 34 outflow: a possible jet deceleration mechanism. Astrophysical Journal. 2002 ; 580 950-958. -
Vancouver
Masciadri E, Gouveia dal Pino EM de, Raga AC, Noriega-Crespo A. Precession of the Giant HH 34 outflow: a possible jet deceleration mechanism. Astrophysical Journal. 2002 ; 580 950-958. - MHD instabilities in accretion disks and their implications in driving fast magnetic reconnection
- Ambient effects on astrophysical jets
- Efeitos de campos magnéticos na estrutura de jatos cósmicos
- Qual a origem dos fluxos moleculares bipolares ?
- Nature of wiggling jets
- Stability and collimation of three-dimensional spmhd jets
- Three-dimensional simulations of protostellar jets in stratified ambient media
- Origin of internal knots in astrophysical jets revised in the light of 3-d numerical simulations
- Numerical simulations of protostellar wiggling jets
- Magnetic reconnection and Blandford–Znajek process around rotating black holes
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