A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations (2018)

First Author: Cantiello M
Attributed to:  Astrophysics Research at the University of Leicester funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.3847/2041-8213/aaad64

Publication URI: http://dx.doi.org/10.3847/2041-8213/aaad64

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 2