Shock-Cloud Interaction in RX J1713.7−3946 Evidence for Cosmic-Ray Acceleration in the Young VHE γ-ray Supernova Remnant

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 int...

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Bibliographic Details
Main Author: Sano, Hidetoshi
Format: eBook
Language:English
Published: Tokyo Springer Japan 2017, 2017
Edition:1st ed. 2017
Series:Springer Theses, Recognizing Outstanding Ph.D. Research
Subjects:
Online Access:
Collection: Springer eBooks 2005- - Collection details see MPG.ReNa
Table of Contents:
  • 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