A Numerical Code to Study the Variability of Blazar Emission (Poster)

Details A Numerical Code to Study the Variability of Blazar Emission (Poster) A Numerical Code to Study the Variability of Blazar Emission (Poster)

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003heba.conf..167t&link_type=abstract

High Energy Blazar Astronomy, ASP Conference Proceedings, Vol. 299, held 17-21 June 2002 at Tuorla Observatory, Piikkio, Finland

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We present a numerical code, written in C, which can be used to simulate or to analyze the emission of Blazars over the entire electromagnetic spectrum. Our code can reproduce the following features: Synchrotron emission. (Inoue & Takahara 1996 ),(Rybicki & Lightman 1979) - Inverse Compton emission (Thomson & Klein-Nishina regime). (Band & Grindlay 1985),(Blumenthal & Gould 1970) - External Compton emission. - Accretion Disk variability using a Cellular Automata algorithm. - Temporal evolution of the emitting plasma energy distribution. - Flaring phenomena. - Light curves in the rest and in the Observer frame (taking account for time crossing effects) In the following pages, we present the results obtained by our code.

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