An Optically-Thin Strong Magnetic Field Model for the Energy Distribution and Time-Variability of Blazars

Details An Optically-Thin Strong Magnetic Field Model for the Energy Distribution and Time-Variability of Blazars An Optically-Thin Strong Magnetic Field Model for the Energy Distribution and Time-Variability of Blazars

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986rmxaa..12...53l&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, 12, 53

Astronomy and Astrophysics

Astronomy

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1986RMxAA..12...53L

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