Gamma-ray flux distribution and nonlinear behavior of four lat bright AGNs (2017)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- DOI: 10.3847/1538-4357/aa8ef5
- Subjects: BURACOS NEGROS; GALÁXIAS ATIVAS; RAIOS GAMA
- Language: Inglês
- Imprenta:
- Source:
- Título: Astrophysical Journal
- ISSN: 0004-637X
- Volume/Número/Paginação/Ano: v. 849, p. 138, 2017
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
-
ABNT
KUSHWAHA, Pankaj et al. Gamma-ray flux distribution and nonlinear behavior of four lat bright AGNs. Astrophysical Journal, v. 849, p. 138, 2017Tradução . . Disponível em: https://arxiv.org/pdf/1709.07904.pdf. Acesso em: 10 jan. 2026. -
APA
Kushwaha, P., Sinha, A., Misra, R., & Dal Pino, E. M. de G. (2017). Gamma-ray flux distribution and nonlinear behavior of four lat bright AGNs. Astrophysical Journal, 849, 138. doi:10.3847/1538-4357/aa8ef5 -
NLM
Kushwaha P, Sinha A, Misra R, Dal Pino EM de G. Gamma-ray flux distribution and nonlinear behavior of four lat bright AGNs [Internet]. Astrophysical Journal. 2017 ; 849 138.[citado 2026 jan. 10 ] Available from: https://arxiv.org/pdf/1709.07904.pdf -
Vancouver
Kushwaha P, Sinha A, Misra R, Dal Pino EM de G. Gamma-ray flux distribution and nonlinear behavior of four lat bright AGNs [Internet]. Astrophysical Journal. 2017 ; 849 138.[citado 2026 jan. 10 ] Available from: https://arxiv.org/pdf/1709.07904.pdf - Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection
- Prospect on intergalactic magnetic field measurements with gamma-ray instruments
- A magnetic reconnection model for explaining the multiwave length emission of the microquasars Cyg X-1 and Cyg X-3
- 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
- The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks
Informações sobre o DOI: 10.3847/1538-4357/aa8ef5 (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
