Add to ORKGIf cosmic rays with energies 500 GeV flux are reported. Non-thermal X-ray emission detected from one of these remnants (Cassiopeia A) has been interpreted as synchrotron emission from electrons in the ambient magnetic fields. Gamma-ray emission detected from the Monoceros/Rosette Nebula region has been interpreted as evidence of cosmic-ray acceleration. We interpret our results in the context of these observations
It is widely believed that the bulk of the Galactic cosmic rays are accelerated in supernova remnant...
Supernova remnants (SNRs) are widely believed to be the principal source of galactic cosmic rays. Su...
Diffusive shock acceleration operating at expanding supernova remnant shells is by far the most popu...
If cosmic rays with energies 500 GeV flux are reported. Non-thermal X-ray emission detected from one...
If supernova remnants (SNRs) are the sites of cosmic-ray acceleration, the associated nuclear intera...
We report the results of TeV gamma-ray observations of the shell type SNR RXJ1713.7-3946 (G347.3-0.5...
The observation by the CANGAROO experiment of TeV emission from SN 1006, in conjunction with several...
This paper reports the first discovery of TeV gamma-ray emission from a supernova remnant made with ...
Combining archival data taken at radio and infrared wavelengths with state-of-the-art measurements a...
In this Letter we report the discovery of TeV gamma-ray emission from a supernova remnant made with ...
Galactic cosmic rays are believed to be accelerated at supernova remnant shocks. Though very popular...
232 hours of data were accumulated from 1997 to 1999, using the HEGRA Stereoscopic Cherenkov Telesco...
The origin of Galactic cosmic rays is still a burning question that forms a major motivation for dev...
We report the results of TeV gamma-ray observations of the shell type SNR RXJ1713.7-3946 (G347.3-0.5...
A number of nearby northern hemisphere shell-type supernova remnants (SNRs) has been observed in TeV...
It is widely believed that the bulk of the Galactic cosmic rays are accelerated in supernova remnant...
Supernova remnants (SNRs) are widely believed to be the principal source of galactic cosmic rays. Su...
Diffusive shock acceleration operating at expanding supernova remnant shells is by far the most popu...
If cosmic rays with energies 500 GeV flux are reported. Non-thermal X-ray emission detected from one...
If supernova remnants (SNRs) are the sites of cosmic-ray acceleration, the associated nuclear intera...
We report the results of TeV gamma-ray observations of the shell type SNR RXJ1713.7-3946 (G347.3-0.5...
The observation by the CANGAROO experiment of TeV emission from SN 1006, in conjunction with several...
This paper reports the first discovery of TeV gamma-ray emission from a supernova remnant made with ...
Combining archival data taken at radio and infrared wavelengths with state-of-the-art measurements a...
In this Letter we report the discovery of TeV gamma-ray emission from a supernova remnant made with ...
Galactic cosmic rays are believed to be accelerated at supernova remnant shocks. Though very popular...
232 hours of data were accumulated from 1997 to 1999, using the HEGRA Stereoscopic Cherenkov Telesco...
The origin of Galactic cosmic rays is still a burning question that forms a major motivation for dev...
We report the results of TeV gamma-ray observations of the shell type SNR RXJ1713.7-3946 (G347.3-0.5...
A number of nearby northern hemisphere shell-type supernova remnants (SNRs) has been observed in TeV...
It is widely believed that the bulk of the Galactic cosmic rays are accelerated in supernova remnant...
Supernova remnants (SNRs) are widely believed to be the principal source of galactic cosmic rays. Su...
Diffusive shock acceleration operating at expanding supernova remnant shells is by far the most popu...