Does the SN rate explain the very high energy cosmic rays in the central 200 pc of our Galaxy?
Does the SN rate explain the very high energy cosmic rays in the central 200 pc of our Galaxy?
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Author / Creator
Jouvin, L , Lemière, A and Terrier, R
Publisher
Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
The H.E.S.S. collaboration revealed the presence of a very high energy (VHE) diffuse emission in the inner 100pc of the Galaxy in close correlation with the Central Molecular Zone (CMZ). Recently, they deduced from this emission a cosmic-ray (CR) over-density in the region with a local peak toward the Galactic Center (GC) and proposed a diffusive s...
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Full title
Does the SN rate explain the very high energy cosmic rays in the central 200 pc of our Galaxy?
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TN_cdi_proquest_journals_2074461092
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2074461092
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1703.10398
