Possible mechanism for radio and gamma-ray emissions in accreting black hole sources (2015)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- Subjects: RAIOS GAMA; BURACOS NEGROS
- Language: Inglês
- Imprenta:
- Publisher: International Astronomical Union
- Publisher place: Paris
- Date published: 2015
- Source:
- Título do periódico: Meeting Abstracts
- Conference titles: IAU General Assembly
-
ABNT
DAL PINO, Elisabete Maria de Gouveia e SINGH, C. B e KADOWAKI, L. Possible mechanism for radio and gamma-ray emissions in accreting black hole sources. 2015, Anais.. Paris: International Astronomical Union, 2015. . Acesso em: 11 maio 2024. -
APA
Dal Pino, E. M. de G., Singh, C. B., & Kadowaki, L. (2015). Possible mechanism for radio and gamma-ray emissions in accreting black hole sources. In Meeting Abstracts. Paris: International Astronomical Union. -
NLM
Dal Pino EM de G, Singh CB, Kadowaki L. Possible mechanism for radio and gamma-ray emissions in accreting black hole sources. Meeting Abstracts. 2015 ;[citado 2024 maio 11 ] -
Vancouver
Dal Pino EM de G, Singh CB, Kadowaki L. Possible mechanism for radio and gamma-ray emissions in accreting black hole sources. Meeting Abstracts. 2015 ;[citado 2024 maio 11 ] - The effects of magnetic fields on radiative cooling jets
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- Probing magneto-centrifugal scenarios for jet production
- On the production and acceleration of astrophysical jets: a comparative study
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