Optical Monitoring Sample of the GEV Gamma-Ray-loud Blazars

Details Optical Monitoring Sample of the GEV Gamma-Ray-loud Blazars Optical Monitoring Sample of the GEV Gamma-Ray-loud Blazars

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999apj...522..846x&link_type=abstract

The Astrophysical Journal, Volume 522, Issue 2, pp. 846-862.

Astronomy and Astrophysics

Astronomy

51

Galaxies: Bl Lacertae Objects: General, Gamma Rays: Observations, Radiation Mechanism: Nonthermal

Scientific paper

We present optical monitoring between 1994 February and 1997 December of 10 gamma-ray-loud blazars included in our blazar monitoring program. Most of the monitored objects show significant rapid variations. The typical minimum variability timescale in the optical range is about 1 hour. We have analyzed the relationships between optical variability and gamma-ray variability, and discussed theoretical models for the gamma-ray-loud blazar emission.

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