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Shock-Cloud Interaction in RX J1713.7 3946
- Evidence for Cosmic-Ray Acceleration in the Young VHE -ray Supernova Remnant
part of the Springer Theses series
- Binding:
- Paperback
- Pages:
- 134
- Published:
- June 28, 2018
- Edition:
- 12017
- Dimensions:
- 155x235x0 mm.
- Weight:
- 454 g.
Delivery:
1-2 weeks
Expected delivery: December 6, 2024
Description of Shock-Cloud Interaction in RX J1713.7 3946
This book presents a study of the young supernova remnant RX J1713.7-3946 in order to reveal the origin of cosmic rays in our galaxy. The book reveals that the interstellar gas plays an essential role in producing the high-energy radiation and cosmic rays, offering vital new insights into the origin and behavior of galactic cosmic rays.
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