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Compton Gamma-Ray Observatory Science Support Center

EGRET Image of the Blazar 3C279

EGRET Image of the Blazar 3C279

This EGRET image shows the gamma-ray quasars 3C279 and 3C273. Prior to the launch of the Compton Observatory in June of 1991, the quasar 3C273 was the only extragalactic source of high-energy gamma-rays known. However, when the EGRET instrument viewed this region of the sky, they discovered another quasar, 3C279, to be brighter than 3C273. In fact, 3C279 was one of the brightest high-energy gamma-ray objects in the sky in June 1991. This is all-the-more remarkable considering its tremendous distance of about 4 billion light years. 3C279 is now considered to be the archetypical member of a new class of active galaxies discovered by EGRET known as blazars.

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This page was last modified on Monday, 01-Aug-2005 13:41:42 EDT.

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