Supernova Origin of Cosmic Rays from a γ -Ray Signal in the Constellation III Region of the Large Magellanic Cloud-Reference-Cited by-同舟云学术

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Supernova Origin of Cosmic Rays from a γ -Ray Signal in the Constellation III Region of the Large Magellanic Cloud

Published:2017-11-06 Issue:19 Volume:119 Page:
ISSN:0031-9007
Container-title:Physical Review Letters
language:en
Short-container-title:Phys. Rev. Lett.

Author:

Neronov Andrii

Publisher

American Physical Society (APS)

Subject

General Physics and Astronomy

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.119.191102/fulltext

Reference31 articles.

1. On the Origin of the Cosmic Radiation

2. The acceleration of cosmic rays in shock fronts - II

3. Cosmic Rays from Super-Novae

4. Origin of Cosmic Rays

Cited by 9 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Unveiling the nature of the unidentified gamma-ray sources 4FGL J1908.6+0915e, HESS J1907+089/HOTS J1907+091, and 3HWC J1907+085 in the sky region of the magnetar SGR 1900+14;Monthly Notices of the Royal Astronomical Society;2022-05-11

2. Simulating TeV gamma-ray morphologies of shell-type supernova remnants;Monthly Notices of the Royal Astronomical Society;2020-09-18

3. Extremely High Energy (E > 1020 eV) Cosmic Rays: Potential Sources;Kinematics and Physics of Celestial Bodies;2020-05

4. Extremely high energy (E > 1020 eV) cosmic rays: potential sources;Kinematika i fizika nebesnyh tel (Online);2020-05-01

5. Cosmic ray models;Progress in Particle and Nuclear Physics;2019-11

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