ausblenden:
Schlagwörter:
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Zusammenfassung:
The on-going H.E.S.S. Galactic Plane Survey continues to reveal new sources of VHE g -rays. In
particular, recent re-observations of the region around the shell-type supernova remnant (SNR)
G318.2+0.1 have resulted in the discovery of statistically-significant very-high-energy (VHE) g -
ray emission from an extended region. Although the source remains unidentified, archival observations
of 12CO in the region provide an opportunity to investigate a potential SNR/molecular
cloud interaction. The morphological properties of this newly-discovered VHE g -ray source
HESSJ1457−593 are presented and discussed in light of the multi-wavelength data available.