Rodríguez-Ramírez, Juan Carlos 
; Dal Pino, Elisabete Maria de Gouveia ; Batista, Rafael Alves
Source: The Astrophysical Journal. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, MAGNETOHIDRODINÂMICA, CENTRO GALÁCTICO
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RODRÍGUEZ-RAMÍREZ, Juan Carlos e DAL PINO, Elisabete Maria de Gouveia e BATISTA, Rafael Alves. Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*}. The Astrophysical Journal, v. 879, n. 1, p. 6/1-6/10, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab212e. Acesso em: 05 nov. 2024.APA
Rodríguez-Ramírez, J. C., Dal Pino, E. M. de G., & Batista, R. A. (2019). Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*}. The Astrophysical Journal, 879( 1), 6/1-6/10. doi:10.3847/1538-4357/ab212eNLM
Rodríguez-Ramírez JC, Dal Pino EM de G, Batista RA. Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*} [Internet]. The Astrophysical Journal. 2019 ; 879( 1): 6/1-6/10.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab212eVancouver
Rodríguez-Ramírez JC, Dal Pino EM de G, Batista RA. Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*} [Internet]. The Astrophysical Journal. 2019 ; 879( 1): 6/1-6/10.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab212e
