Abstract
The EGRET telescope detected dozens of Galactic sources at GeV energies, most of which were not firmly identified at the end of the mission. Multi-wavelength studies at radio, X-ray, and TeV wavelengths have discovered probable counterparts to many of these sources. We provide an overview of the observational properties of these Galactic sources which emit across 19 orders of magnitude of the electromagnetic spectrum....
Original language | Undefined |
---|---|
State | Published - Mar 2008 |