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 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: 08 fev. 2023. -
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 2023 fev. 08 ] 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 2023 fev. 08 ] Available from: https://arxiv.org/pdf/1709.07904.pdf - Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations
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Informações sobre o DOI: 10.3847/1538-4357/aa8ef5 (Fonte: oaDOI API)
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