Radio properties of Very High Energy gamma-ray sources

Details Radio properties of Very High Energy gamma-ray sources Radio properties of Very High Energy gamma-ray sources

2009-06-03

arxiv.org/abs/0906.0705v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

7 pages, 1 figure. Invited talk at the International Workshop: "The Low-Frequency Radio Universe", Pune, 8-12 December 2008

Scientific paper

Radio observations of very high energy (VHE) gamma-ray sources are fundamental to identify and reveal their nature, as well as to understand the physics behind these energetic sources. I will comment on some characteristics of extragalactic sources detected at TeV energies and radio wavelengths, and galactic sources such as gamma-ray binaries, supernova remnants (SNRs), or pulsar wind nebulae (PWNs). Special emphasis will be put on unidentified extended TeV sources, in which deep radio observations can severely constrain the proposed models and shed light on the possible sources powering the TeV emission.

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