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Focusing on the supernova remnant RX J1713.7-3946, the study explores the origins of cosmic rays in our galaxy through X-ray and gamma radiation from cosmic ray particles. Utilizing data from the NANTEN2 radio telescope, it reveals a strong correlation between gamma rays and interstellar gas, providing evidence for the acceleration of cosmic ray protons. The author highlights the significance of "shock-cloud interaction" between supernova shockwaves and interstellar gas in enhancing cosmic ray electron acceleration, offering new insights into high-energy radiation and cosmic ray behavior.
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Shock-Cloud Interaction in RX J1713.7-3946, Hidetoshi Sano
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- Released
- 2016
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- (Hardcover)
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