A continuous monitoring of the Galactic Centre region has been performed with the WFC~s on board BeppoSAX on a time spread of about 7 months for a total of 500 ks exposure time. The long repeated observations allowed for the identification of 14 bursting sources, 2 of which uncataloged (SAXJ1750-290
β¦ LIBER β¦
The H.E.S.S. view of the Galactic Centre region
β Scribed by Christopher van Eldik
- Publisher
- Elsevier Science
- Year
- 2008
- Tongue
- English
- Weight
- 390 KB
- Volume
- 588
- Category
- Article
- ISSN
- 0168-9002
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β¦ Synopsis
Measurements by High Energy Stereoscopic System (H.E.S.S.) provide the first sensitive map of very-high-energy (VHE) g-ray emission from the central few hundred parsecs of our galaxy. These observations are a valuable tool to understand the acceleration and propagation of energetic particles near the Galactic Centre (GC). The data reveal the existence of three discrete VHE g-ray sources and the presence of diffuse g-ray emission correlated with dense molecular clouds.
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