Könyv Shock-Cloud Interaction in RX J1713.7 3946 Hidetoshi Sano

Shock-Cloud Interaction in RX J1713.7 3946

Evidence for Cosmic-Ray Acceleration in the Young VHE -ray Supernova Remnant

Szerző: Hidetoshi Sano
Nyelv: Angol
Kötés: Kemény kötésű
Elérhetőség: Beszállítói készleten alacsony példányszámban
Küldés 13-18 napon belül
41 425 Ft
This book presents a study of the young supernova remnant RX J1713.7-3946 in order to reveal the ori...

Információk a könyvről

Szerző
Nyelv
Angol
Kötés
Könyv - Kemény kötésű
Kiadva
2016
oldal
134
EAN
9784431556350
ISBN
4431556354
Enbook ID
09256134
Súly
3495
Méretek
155 x 235 x 12

Teljes leírás

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 is focusing on the X-ray and gamma-radiation from the cosmic-ray electrons and/or 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.

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