Simulations of time-dependent high energy emission from blazars

Details Simulations of time-dependent high energy emission from blazars Simulations of time-dependent high energy emission from blazars

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..556..119k&link_type=abstract

EXPLOSIVE PHENOMENA IN ASTROPHYSICAL COMPACT OBJECTS: First KIAS Astrophysics Workshop. AIP Conference Proceedings, Volume 556,

Astronomy and Astrophysics

Astrophysics

Active And Peculiar Galaxies And Related Systems, Radiation Mechanisms, Polarization

Scientific paper

Blazars are a group of active galactic nuclei which emit a broad band continuum from radio to very high energy gamma-rays. Recent X-ray and gamma-ray observations show that the emission from blazars are variable on very short timescales. Based on the synchrotron-self-Compton model for emission mechanisms in relativistic jets, we show the results of the numerical simulations of the time evolution of electron and photon spectra in the jets of blazars, including the effect of electron acceleration. .

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