Evidence that the maximum electron energy in hotspots of FR II galaxies is not determined by synchrotron cooling (2016)

First Author: Araudo A
Attributed to:  Astrophysics and Planetary Science at Oxford 2013-16 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stw1204

Publication URI: http://dx.doi.org/10.1093/mnras/stw1204

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 4

ISSN: 0035-8711