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 do periódico: 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; SINHA, Atreyee; MISRA, Ranjeev; DAL PINO, Elisabete Maria de Gouveia. Gamma-ray flux distribution and nonlinear behavior of four lat bright AGNs. Astrophysical Journal, Bristol, v. 849, p. 138, 2017. Disponível em: < https://arxiv.org/pdf/1709.07904.pdf > DOI: 10.3847/1538-4357/aa8ef5. -
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.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.Available from: https://arxiv.org/pdf/1709.07904.pdf - Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations
- Magnetic reconnection and Blandford–Znajek process around rotating black holes
- The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays
- Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations
- Acceleration of energetic particles through reconnection of weakly stochastic magnetic field
- MHD instabilities in accretion disks and their implications in driving fast magnetic reconnection
- Multiwavelength temporal and spectral variability of the blazar OJ 287 during and after the 2015 December flare: a major accretion disc contribution
- Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs
- Constraints on the production of ultra-high-energy cosmic-rays in compact sources with strong magnetic fields
- 3-d sph simulations of hd and mhd jets
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
