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γ-ray emission from PWNe interacting with molecular clouds

✍ Scribed by H. Bartko; W. Bednarek


Book ID
110842659
Publisher
John Wiley and Sons
Year
2008
Tongue
English
Weight
105 KB
Volume
385
Category
Article
ISSN
0035-8711

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Cosmic rays up to at least 10 15 eV (PeV) are believed to be emitted by Galactic sources, such as supernova remnants. However, no conclusive evidence of their acceleration has been found yet. A trace of ongoing cosmic-ray acceleration is the gamma-ray emission produced by these highly energetic part