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Searches for Tev γ-Ray Emission with the Hegra Cherenkov Telescopes

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Astrophysical Sources of High Energy Particles and Radiation

Part of the book series: NATO Science Series ((NAII,volume 44))

Abstract

Searches for Galactic and extragalactic sources of TeV γ-rays are described using the HEGRA stereoscopic system of imaging atmospheric Cherenkov telescopes with its good angular resolution and γ-hadron separation capability. We present results from recent observations of the interaction region of the Monoceros supernova remnant and the Rosette nebula, from the young open star clusters Berkeley 87 and IC 1805, and the giant radiogalaxies M 87, NGC 1275 and Cygnus A. Upper flux limits with energy thresholds between 0.7 and 1.2 TeV are obtained in the range of 0.5 to 2.5 x 10-12ph.cm-2s-1 for the individual objects.

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© 2001 Springer Science+Business Media Dordrecht

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Götting, N., Lucarelli, F., Tluczykont, M. (2001). Searches for Tev γ-Ray Emission with the Hegra Cherenkov Telescopes. In: Shapiro, M.M., Stanev, T., Wefel, J.P. (eds) Astrophysical Sources of High Energy Particles and Radiation. NATO Science Series, vol 44. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0560-9_18

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  • DOI: https://doi.org/10.1007/978-94-010-0560-9_18

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-1-4020-0174-1

  • Online ISBN: 978-94-010-0560-9

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