EVOLUTION OF HIGH-ENERGY PARTICLE DISTRIBUTION IN MATURE SHELL-TYPE SUPERNOVA REMNANTS

EVOLUTION OF HIGH-ENERGY PARTICLE DISTRIBUTION IN MATURE SHELL-TYPE SUPERNOVA REMNANTS

Multi-wavelength observations of mature supernova remnants (SNRs), especially with recent advances in gamma-ray astronomy, make it possible to constrain energy distribution of energetic particles within these remnants. In consideration of the SNR origin of Galactic cosmic rays and physics related to...

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Bibliographic Details
Main Authors: Zeng, Houdun, Xin, Yuliang, Liu, Siming, Jokipii, J. R., Zhang, Li, Zhang, Shuinai
Other Authors: Univ Arizona
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
cosmic rays
gamma rays: ISM
ISM: supernova remnants
radiation mechanisms: non-thermal
Online Access:http://hdl.handle.net/10150/623101
http://arizona.openrepository.com/arizona/handle/10150/623101

Internet

http://hdl.handle.net/10150/623101
http://arizona.openrepository.com/arizona/handle/10150/623101

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