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The acceleration of cosmic-ray protons in the supernova remnant RX J1713.7–3946

✍ Scribed by Enomoto, R.; Tanimori, T.; Naito, T.; Yoshida, T.; Yanagita, S.; Mori, M.; Edwards, P. G.; Asahara, A.; Bicknell, G. V.; Gunji, S.


Book ID
109803435
Publisher
Nature Publishing Group
Year
2002
Tongue
English
Weight
280 KB
Volume
416
Category
Article
ISSN
0028-0836

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Arguments against a dominantly hadronic
✍ R. Plaga 📂 Article 📅 2008 🏛 Elsevier Science 🌐 English ⚖ 133 KB

The flux of photons above 1 TeV from the direction of the centre and a cloud in the western part of the nearby southern supernova remnant (SNR) RX J1713.7-3946 is calculated in the ''hadronic scenario'' that aims to explain the intense VHE radiation from this remnant with the decay of p 0 pions prod