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Conference Paper

Discovery of VHE gamma-rays from the vicinity of the shell-type SNR G318.2+0.1 with H.E.S.S.

MPS-Authors
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Hofverberg,  Petter
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Chaves,  Ryan Carlos Goncalves
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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de Ona Wilhelmi,  Emma
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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http://pos.sissa.it/archive/conferences/123/196/Texas%202010_196.pdf
(Publisher version)

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Citation

Hofverberg, P., Chaves, R. C. G., Fiasson, A., Kosack, K., Mehault, J., de Ona Wilhelmi, E., et al. (2011). Discovery of VHE gamma-rays from the vicinity of the shell-type SNR G318.2+0.1 with H.E.S.S. Proceedings of Science, Texas2010: 196, 1-7.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0012-3247-D
Abstract
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.