Evidence for X-ray Emission in Excess to the Jet Afterglow Decay 3.5 yrs After the Binary Neutron Star Merger GW 170817: A New Emission Component (2021)
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.2104.02070
Publication URI: https://arxiv.org/abs/2104.02070
Type: Other