VERITAS observations of M87

ORAL

Abstract

M87 is a giant radio galaxy located at 16Mpc away and is observed from radio to TeV gamma-rays. Its jet features are well studied in radio, optical, and X-ray. The proximity of M87 provides a unique opportunity for multi-wavelength observations to study the source and mechanisms of high energy emission from active galactic nuclei. The VERITAS atmospheric Cherenkov telescope array detected gamma-ray emission above 250GeV from M87 in 2007 and 2008. The 2008 observation was part of a long-term monitoring study coordinated between 3 TeV gamma-ray experiments, H.E.S.S., MAGIC, and VERITAS, resulting in the detection of multiple TeV flares. The monitoring campaign is continued in 2009 and we will present preliminary results from VERITAS observation.

Authors

  • Chiumun Michelle Hui

    University of Utah