The Full Spectrum Galactic Terrarium: MHz to TeV Observations of Various Critters

Details The Full Spectrum Galactic Terrarium: MHz to TeV Observations of Various Critters The Full Spectrum Galactic Terrarium: MHz to TeV Observations of Various Critters

2008-11-04

arxiv.org/abs/0811.0570v1

Astronomy and Astrophysics

Astrophysics

4 pages, 5 figures, Proceedings of the The 4th Heidelberg International Symposium on High Energy Gamma-Ray Astronomy, eds. Aha

Scientific paper

10.1063/1.3076673

Multi-wavelength studies at radio, infrared, optical, X-ray, and TeV wavelengths have discovered probable counterparts to many Galactic sources of GeV emission detected by EGRET. These include pulsar wind nebulae, high mass X-ray binaries, and mixed morphology supernova remnants. Here we provide an overview of the observational properties of Galactic sources which emit across 19 orders of magnitude in energy. We also present new observations of several sources.

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