Intranight Variability of Blazar Mrk180

Details Intranight Variability of Blazar Mrk180 Intranight Variability of Blazar Mrk180

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010fym..confp..43a&link_type=abstract

"The First Year of MAXI: Monitoring Variable X-ray Sources", Poster Presentations, 4th International MAXI Workshop held November

Physics

Scientific paper

Blazars vary at all wavelengths over a variety of timescales. Various models have been proposed to explain blazar variability, however, the mechanism responsible for variability is not conclusively understood. One factor which can discriminate among the various variability models is that of colour (spectral index) variations of blazars. By this one may be able to better understand the mechanism of blazar variability. It is also, currently inconclusive if all blazars have similar spectral variability nature. We have therefore carried out quasi-simultaneous multiband monitoring of one of the brightest GeV blazar, Mrk 180, on 23 Apr 2009. We will present the results of intranight variability.

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