The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks (2012)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- DOI: 10.1088/0004-637X/747/1/21
- Subjects: DISCOS DE ACRESÇÃO; MEIO INTERESTELAR; CAMPO MAGNÉTICO; MAGNETOHIDRODINÂMICA; FORMAÇÃO DE ESTRELAS; TURBULÊNCIA
- Language: Inglês
- Imprenta:
- Source:
- Título: The Astrophysical Journal
- ISSN: 0004-637X
- Volume/Número/Paginação/Ano: v. 747, p. 21/1-21/8, 2012
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
-
ABNT
SANTOS-LIMA, R e DAL PINO, Elisabete Maria de Gouveia e LAZARIAN, A. The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks. The Astrophysical Journal, v. 747, p. 21/1-21/8, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/747/1/21. Acesso em: 11 jan. 2026. -
APA
Santos-Lima, R., Dal Pino, E. M. de G., & Lazarian, A. (2012). The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks. The Astrophysical Journal, 747, 21/1-21/8. doi:10.1088/0004-637X/747/1/21 -
NLM
Santos-Lima R, Dal Pino EM de G, Lazarian A. The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks [Internet]. The Astrophysical Journal. 2012 ; 747 21/1-21/8.[citado 2026 jan. 11 ] Available from: https://doi.org/10.1088/0004-637X/747/1/21 -
Vancouver
Santos-Lima R, Dal Pino EM de G, Lazarian A. The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks [Internet]. The Astrophysical Journal. 2012 ; 747 21/1-21/8.[citado 2026 jan. 11 ] Available from: https://doi.org/10.1088/0004-637X/747/1/21 - Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection
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Informações sobre o DOI: 10.1088/0004-637X/747/1/21 (Fonte: oaDOI API)
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