Microvariability in Blazars

Details Microvariability in Blazars Microvariability in Blazars

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21642011w&link_type=abstract

American Astronomical Society, AAS Meeting #216, #420.11

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Scientific paper

We present the results of a long term blazar microvariability program carried out at the SARA observatory since 2004. We calculate the duty cycles for microvariability, discuss the lack of correlations with brightness level, and other analysis of the detailed microvariability curves of 14 Blazars. We discuss the results based on a shot model where the microvariations are the result of shock-heated turbulent cells cooling by synchrotron emission.

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