A magnetic reconnection model for explaining the multiwave length emission of the microquasars Cyg X-1 and Cyg X-3 (2015)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- DOI: 10.1093/mnras/stv248
- Subjects: ACELERAÇÃO DE PARTÍCULAS; MAGNETISMO; RAIOS CÓSMICOS; BURACOS NEGROS
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v. 449, p. 34–48, 2015
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
ABNT
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: 12 jan. 2026. -
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/stv248 -
NLM
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 2026 jan. 12 ] Available from: https://doi.org/10.1093/mnras/stv248 -
Vancouver
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 2026 jan. 12 ] Available from: https://doi.org/10.1093/mnras/stv248 - Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection
- Prospect on intergalactic magnetic field measurements with gamma-ray instruments
- Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not?
- Multiwavelength temporal and spectral variability of the blazar OJ 287 during and after the 2015 December flare: a major accretion disc contribution
- 3D hydrodynamical simulations of galactic winds: an application to the starburst galaxy M82
- The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays
- Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs
- Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations
- Gamma-ray flux distribution and nonlinear behavior of four lat bright AGNs
- The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks
Informações sobre o DOI: 10.1093/mnras/stv248 (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
