Very high energy gamma rays from the direction of Sagittarius A

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Abstract

We report the detection of a point-like source of very high energy (VHE) γ-rays coincident within 1′ of Sgr A*, obtained with the HESS array of Cherenkov telescopes. The γ-rays exhibit a power-law energy spectrum with a spectral index of -2.2 ± 0.09 × 0.15 and a flux above the 165 GeV threshold of (1.82 ± 0.22) × 10-7 m-2 s-1. The measured flux and spectrum differ substantially from recent results reported in particular by the CANGAROO collaboration.

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Aharonian, F., Akhperjanian, A. G., Aye, K. M., Bazer-Bachi, A. R., Beilicke, M., Benbow, W., … Wagner, S. J. (2004). Very high energy gamma rays from the direction of Sagittarius A. Astronomy and Astrophysics, 425(1). https://doi.org/10.1051/0004-6361:200400055

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