Did Egret Detect Distant Supernova Remnants?
arXiv:astro-ph/0301424 · doi:10.1016/j.asr.2003.07.031
Abstract
It might be thought that supernova remnants (SNRs) more distant than a few kiloparsec from Earth could not have been detected by the EGRET experiment. This work analyzes the observational status of this statement in the light of new CO studies of SNRs.
Accepted for publication in Advances in Space Research, in High Energy Studies of Supernova Remnants and Neutron Stars, eds. W. Becker and W. Hermsen (2003)
References in corpus (17)
- The Milky Way in Molecular Clouds: A New Complete CO Survey
- A New Relation and Its Application to the Galactic Supernova Remnant Distribution
- X-Ray Emission From the Shell-Type SNR G347.3-0.5
- PSR J2229+6114: Discovery of an Energetic Young Pulsar in the Error Box of the EGRET Source 3EG J2227+6122
- Supernova remnants and gamma-ray sources
- Shock-Excited Maser Emission from Supernova Remnants: G32.8-0.1, G337.8-0.1, G346.6-0.2, and the HB3/W3 Complex
- A variability analysis of low-latitude unidentified gamma-ray sources
- Supernova-Remnant Origin of Cosmic Rays?
- Multiwavelength Examination of the COS-B Field 2CG 075+00 Yields a Blazar Identification for 3EG J2016+3657
- Testing the Correlation of Ultra-High Energy Cosmic Rays with High Redshift Sources
- Recently discovered pulsars and unidentified EGRET sources
- Is the Supernova Remnant RX J1713.7-3946 a Hadronic Cosmic Ray Accelerator ?
- 3EG J2016+3657: Confirming an EGRET Blazar Behind the Galactic Plane
- An Asca Study of the Supernova Remnant G39.2-0.3
- Evidence for TeV gamma-ray emission from the shell type SNR RXJ1713.7-3946
- Applications of Likelihood Analysis in Gamma-Ray Astrophysics
- Unidentified 3EG gamma-ray sources at low galactic latitude