Shock-Cloud Interaction in RX J1713.7−3946
Evidence for Cosmic-Ray Acceleration in the Young VHE γ-ray Supernova Remnant
Seiten
2018
|
Softcover reprint of the original 1st ed. 2017
Springer Verlag, Japan
978-4-431-56673-1 (ISBN)
Springer Verlag, Japan
978-4-431-56673-1 (ISBN)
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.
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 study focuses on the X-ray and gamma radiation from the cosmic ray electrons and protons in the supernova remnant as well as the emission from the surrounding interstellar gas measured by the NANTEN2 4-m radio telescope at Nagoya University. The gamma rays show a good spatial correspondence with the interstellar gas, which for the first time provides strong evidence of the acceleration of cosmic ray protons. Additionally, the author determines that an interaction between the supernova shockwaves and interstellar gas, referred to as “shock-cloud interaction,” promotes the efficient acceleration of cosmic ray electrons in the supernova remnant. 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.
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 study focuses on the X-ray and gamma radiation from the cosmic ray electrons and protons in the supernova remnant as well as the emission from the surrounding interstellar gas measured by the NANTEN2 4-m radio telescope at Nagoya University. The gamma rays show a good spatial correspondence with the interstellar gas, which for the first time provides strong evidence of the acceleration of cosmic ray protons. Additionally, the author determines that an interaction between the supernova shockwaves and interstellar gas, referred to as “shock-cloud interaction,” promotes the efficient acceleration of cosmic ray electrons in the supernova remnant. 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.
Introduction.- Non-Thermal X-ray Enhancement around Dense Gas Clumps.- Evidence for the Acceleration of Cosmic Ray Protons.- Evidence for Efficient Acceleration of Cosmic Rays.- Summary and Future Prospects.
| Erscheinungsdatum | 20.08.2018 |
|---|---|
| Reihe/Serie | Springer Theses |
| Zusatzinfo | 53 Illustrations, color; 7 Illustrations, black and white; XIII, 134 p. 60 illus., 53 illus. in color. |
| Verlagsort | Tokyo |
| Sprache | englisch |
| Maße | 155 x 235 mm |
| Themenwelt | Naturwissenschaften ► Physik / Astronomie ► Astronomie / Astrophysik |
| Naturwissenschaften ► Physik / Astronomie ► Hochenergiephysik / Teilchenphysik | |
| Schlagworte | Cosmic-ray accelerator • Cosmic-ray proton acceleration • Gamma-ray and X-ray astronomy • Interstellar gas shock waves • Interstellar Medium • Radio astronomy NANTEN2 • Shock-cloud interaction • snr • Very high energy gamma-rays • VHE |
| ISBN-10 | 4-431-56673-2 / 4431566732 |
| ISBN-13 | 978-4-431-56673-1 / 9784431566731 |
| Zustand | Neuware |
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