Magnetic reconnection and Blandford–Znajek process around rotating black holes (2018)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- DOI: 10.1093/mnras/sty1405
- Subjects: DISCOS DE ACRESÇÃO; BURACOS NEGROS; RAIOS X
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Monthly Notices of the Royal Astronomical Society
- Volume/Número/Paginação/Ano: v. 478, n. 4, p. 5404-5409, 2018
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
ABNT
SINGH, Chandra B e GAROFALO, David e DAL PINO, Elisabete Maria de Gouveia. Magnetic reconnection and Blandford–Znajek process around rotating black holes. Monthly Notices of the Royal Astronomical Society, v. 478, n. 4, p. 5404-5409, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty1405. Acesso em: 27 jan. 2023. -
APA
Singh, C. B., Garofalo, D., & Dal Pino, E. M. de G. (2018). Magnetic reconnection and Blandford–Znajek process around rotating black holes. Monthly Notices of the Royal Astronomical Society, 478( 4), 5404-5409. doi:10.1093/mnras/sty1405 -
NLM
Singh CB, Garofalo D, Dal Pino EM de G. Magnetic reconnection and Blandford–Znajek process around rotating black holes [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 478( 4): 5404-5409.[citado 2023 jan. 27 ] Available from: https://doi.org/10.1093/mnras/sty1405 -
Vancouver
Singh CB, Garofalo D, Dal Pino EM de G. Magnetic reconnection and Blandford–Znajek process around rotating black holes [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 478( 4): 5404-5409.[citado 2023 jan. 27 ] Available from: https://doi.org/10.1093/mnras/sty1405 - Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations
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Informações sobre o DOI: 10.1093/mnras/sty1405 (Fonte: oaDOI API)
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