Gamma-ray Emission from the Galaxy M87 Observed with VERITAS

Astronomy and Astrophysics – Astronomy

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Scientific paper

The giant radio galaxy M87 is the only extragalactic non-blazar object which has been detected as a source of very high energy gamma-rays. Because of its proximity ( 16 Mpc), it represents a unique opportunity to study in detail the processes occurring in Active Galactic Nuclei from radio to TeV gamma-rays.
In this talk we will report the detection of gamma-ray emission above 250 GeV from M87 in spring 2007 with the VERITAS imaging atmospheric Cherenkov telescope array. We will show the energy spectrum and compare our result to the previous observations with HEGRA and HESS. We will also discuss the X-ray gamma-ray correlation and show strong evidence for a year scale correlation. These results have strong implications for the gamma-ray emitting region in M87.

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