Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not? (2013)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- DOI: 10.1093/mnras/sts597
- Subjects: DISCOS DE ACRESÇÃO; TURBULÊNCIA; MEIO INTERESTELAR; CAMPO MAGNÉTICO
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v. 429. p. 3371-3378, 2013
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
ABNT
SANTOS-LIMA, R e DAL PINO, Elisabete Maria de Gouveia e LAZARIAN, A. Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not?. Monthly Notices of the Royal Astronomical Society, v. 429. p. 3371-3378, 2013Tradução . . Disponível em: https://doi.org/10.1093/mnras/sts597. Acesso em: 04 out. 2024. -
APA
Santos-Lima, R., Dal Pino, E. M. de G., & Lazarian, A. (2013). Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not? Monthly Notices of the Royal Astronomical Society, 429. p. 3371-3378. doi:10.1093/mnras/sts597 -
NLM
Santos-Lima R, Dal Pino EM de G, Lazarian A. Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not? [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 429. p. 3371-3378[citado 2024 out. 04 ] Available from: https://doi.org/10.1093/mnras/sts597 -
Vancouver
Santos-Lima R, Dal Pino EM de G, Lazarian A. Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not? [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 429. p. 3371-3378[citado 2024 out. 04 ] Available from: https://doi.org/10.1093/mnras/sts597 - 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
Informações sobre o DOI: 10.1093/mnras/sts597 (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas