The Feasibility of Magnetic Reconnection Powered Blazar Flares from Synchrotron Self-Compton Emission (2018)
Attributed to:
Astrophysics at Oxford 2016-2019
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1810.04139
Publication URI: https://arxiv.org/abs/1810.04139
Type: Other