Origin of the superluminal ejections in microquasars by violent magnetic reconnection (2003)
- Autores:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- Assunto: MEIO INTERESTELAR
- Idioma: Português
- Imprenta:
- Fonte:
- Título do periódico: Boletim da Sociedade Astronômica Brasileira
- ISSN: 0101-3440
- Volume/Número/Paginação/Ano: v. 23, n.1, p. 42, 2003
- Nome do evento: Reunio Anual da Sociedade Astronômica Brasileira
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ABNT
GOUVEIA DAL PINO, Elisabete Maria de e LAZARIAM, Alex e RAGA, Alex. Origin of the superluminal ejections in microquasars by violent magnetic reconnection. Boletim da Sociedade Astronômica Brasileira. São Paulo: SAB. . Acesso em: 03 jun. 2023. , 2003 -
APA
Gouveia dal Pino, E. M. de, Lazariam, A., & Raga, A. (2003). Origin of the superluminal ejections in microquasars by violent magnetic reconnection. Boletim da Sociedade Astronômica Brasileira. São Paulo: SAB. -
NLM
Gouveia dal Pino EM de, Lazariam A, Raga A. Origin of the superluminal ejections in microquasars by violent magnetic reconnection. Boletim da Sociedade Astronômica Brasileira. 2003 ; 23( 1): 42.[citado 2023 jun. 03 ] -
Vancouver
Gouveia dal Pino EM de, Lazariam A, Raga A. Origin of the superluminal ejections in microquasars by violent magnetic reconnection. Boletim da Sociedade Astronômica Brasileira. 2003 ; 23( 1): 42.[citado 2023 jun. 03 ] - Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations
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