Evidence for X-Ray Emission in Excess to the Jet-afterglow Decay 3.5 yr after the Binary Neutron Star Merger GW 170817: A New Emission Component (2022)

First Author: Hajela A

Attributed to: Astrophysics at Oxford 2016-2019 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.3847/2041-8213/ac504a

Publication URI: http://dx.doi.org/10.3847/2041-8213/ac504a

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal Letters

Issue: 1