A CHANDRA VIEW OF NON-THERMAL EMISSION IN THE NORTHWESTERN REGION OF SUPERNOVA REMNANT RCW 86: PARTICLE ACCELERATION AND MAGNETIC FIELDS

A CHANDRA VIEW OF NON-THERMAL EMISSION IN THE NORTHWESTERN REGION OF SUPERNOVA REMNANT RCW 86: PARTICLE ACCELERATION AND MAGNETIC FIELDS

The shocks of supernova remnants are believed to accelerate particles to cosmic ray (CR) energies. The amplification of the magnetic field due to CRs propagating in the shock region is expected to have an impact on both the emission from the accelerated particle population as well as the acceleratio...

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Bibliographic Details
Main Authors: Castro, Daniel, Lopez, Laura A., Slane, Patrick O., Yamaguchi, Hiroya, Ramirez-Ruiz, Enrico, Figueroa-Feliciano, Enectali
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: Institute of Physics Publishing 2014
Online Access:http://hdl.handle.net/1721.1/88422
https://orcid.org/0000-0002-3243-727X
https://orcid.org/0000-0001-9285-5556

Internet

http://hdl.handle.net/1721.1/88422
https://orcid.org/0000-0002-3243-727X
https://orcid.org/0000-0001-9285-5556

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