Optically-thin, strong magnetic field model for the energy distribution and time-variability of blazars

Optically-thin, strong magnetic field model for the energy distribution and time-variability of blazars (1986)

Authors:
USP affiliated authors: LEPINE, JACQUES RAYMOND DANIEL - IAG ; BRAZ, MARIA ALCINA - IAG
Unidade: IAG
Assunto: ASTRONOMIA
Language: Português
Source:
- Título: Revista Mexicana de Astronomia Y Astrofisica
- Volume/Número/Paginação/Ano: v.12, p.53-8, 1986

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ABNT

LÉPINE, Jacques Raymond Daniel e BRAZ, M A e EPCHTEIN, N. Optically-thin, strong magnetic field model for the energy distribution and time-variability of blazars. Revista Mexicana de Astronomia Y Astrofisica, v. 12, p. 53-8, 1986Tradução . . Acesso em: 25 jan. 2026.
APA

Lépine, J. R. D., Braz, M. A., & Epchtein, N. (1986). Optically-thin, strong magnetic field model for the energy distribution and time-variability of blazars. Revista Mexicana de Astronomia Y Astrofisica, 12, 53-8.
NLM

Lépine JRD, Braz MA, Epchtein N. Optically-thin, strong magnetic field model for the energy distribution and time-variability of blazars. Revista Mexicana de Astronomia Y Astrofisica. 1986 ;12 53-8.[citado 2026 jan. 25 ]
Vancouver

Lépine JRD, Braz MA, Epchtein N. Optically-thin, strong magnetic field model for the energy distribution and time-variability of blazars. Revista Mexicana de Astronomia Y Astrofisica. 1986 ;12 53-8.[citado 2026 jan. 25 ]