@inproceedings{1545fed84eba4221a7ea0a585a9a7bd3,
title = "Pulsars everywhere! A galactic EGRET source retrospective",
abstract = "At the end of the EGRET mission, the only firmly identified sources of GeV emission in our Galaxy were a handful of young pulsars and a solar flare. With the recent launch of AGILE and the imminent launch of GLAST, the sources that EGRET saw will again be studied in γ-rays. We review the multiwavelength observations of the error boxes of Galactic EGRET sources to see what types of sources this new generation of γ-ray telescopes will be studying. I note that most, if not all, of the sources seem to be related to pulsars. Several are probably radio pulsars not known during the time of EGRET. Others are radio-quiet pulsars like Geminga. Still others are probably the product of a pulsar wind interacting with a dense environment. The rest seem to be coincident with things associated with the birth of pulsars i.e. supernova remnants, molecular clouds, and massive star associations.",
keywords = "EGRET, GLAST, Gamma-ray, Pulsar, Pulsar wind nebula, Supernova remnant",
author = "Roberts, {Mallory S.E.}",
year = "2008",
doi = "10.1063/1.2900313",
language = "English (US)",
isbn = "9780735405028",
series = "AIP Conference Proceedings",
pages = "621--623",
booktitle = "40 Years Of Pulsars",
note = "40 Years Of Pulsars: Millisecond Pulsars, Magnetars and More ; Conference date: 12-08-2007 Through 17-08-2007",
}