Observation Of Gamma-Ray Emission From The Galaxy M87 Above 250 Gev With Veritas
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Astrophysics and Astronomy | Physical Sciences and Mathematics
The multiwavelength observation of the nearby radio galaxy M87 provides a unique opportunity to study in detail processes occurring in active galactic nuclei from radio waves to TeV γ-rays. Here we report the detection of γ-ray emission above 250 GeV from M87 in spring 2007 with the VERITAS atmospheric Cerenkov telescope array and discuss its correlation with the X-ray emission. The γ-ray emission is measured to be pointlike with an intrinsic source radius less than 4.5'. The differential energy spectrum is fitted well by a power-law function: dΦ/dE = (7.4 ± 1.3stat ± 1.5sys)(E/TeV)(− 2.31 ± 0.17stat ± 0.2sys) 10−9 m−2 s−1 TeV−1. We show strong evidence for a year-scale correlation between the γ-ray flux reported by TeV experiments and the X-ray emission measured by the ASM RXTE observatory, and discuss the possible short-timescale variability. These results imply that the γ-ray emission from M87 is more likely associated with the core of the galaxy than with other bright X-ray features in the jet.
Reynolds, P. T. and al., Et., "Observation Of Gamma-Ray Emission From The Galaxy M87 Above 250 Gev With Veritas" (2008). Physical Sciences Publications [online].
Available at: https://doi.org/10.1086/587458