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Shock-Cloud Interaction in RX J1713.7 3946: Evidence for Cosmic-Ray Acceleration in the Young VHE -ray Supernova Remnant - Springer Theses 1st ed. 2017 edition
Hidetoshi Sano
Shock-Cloud Interaction in RX J1713.7 3946: Evidence for Cosmic-Ray Acceleration in the Young VHE -ray Supernova Remnant - Springer Theses 1st ed. 2017 edition
Hidetoshi Sano
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.
134 pages, 7 black & white illustrations, 53 colour illustrations, biography
Mídia | Livros Hardcover Book (Livro com lombada e capa dura) |
Lançado | 22 de novembro de 2016 |
ISBN13 | 9784431556350 |
Editoras | Springer Verlag, Japan |
Páginas | 134 |
Dimensões | 155 × 235 × 10 mm · 390 g |
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