Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ACELERAÇÃO DE PARTÍCULAS, MAGNETISMO, RAIOS CÓSMICOS, BURACOS NEGROS
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KHIALI, B e DAL PINO, Elisabete Maria de Gouveia e VALLE, M. V. del. A magnetic reconnection model for explaining the multiwave length emission of the microquasars Cyg X-1 and Cyg X-3. Monthly Notices of the Royal Astronomical Society, v. 449, p. 34–48, 2015Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv248. Acesso em: 14 ago. 2024.APA
Khiali, B., Dal Pino, E. M. de G., & Valle, M. V. del. (2015). A magnetic reconnection model for explaining the multiwave length emission of the microquasars Cyg X-1 and Cyg X-3. Monthly Notices of the Royal Astronomical Society, 449, 34–48. doi:10.1093/mnras/stv248NLM
Khiali B, Dal Pino EM de G, Valle MV del. A magnetic reconnection model for explaining the multiwave length emission of the microquasars Cyg X-1 and Cyg X-3 [Internet]. Monthly Notices of the Royal Astronomical Society. 2015 ; 449 34–48.[citado 2024 ago. 14 ] Available from: https://doi.org/10.1093/mnras/stv248Vancouver
Khiali B, Dal Pino EM de G, Valle MV del. A magnetic reconnection model for explaining the multiwave length emission of the microquasars Cyg X-1 and Cyg X-3 [Internet]. Monthly Notices of the Royal Astronomical Society. 2015 ; 449 34–48.[citado 2024 ago. 14 ] Available from: https://doi.org/10.1093/mnras/stv248
