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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: Warwick Astrophysics Consolidated Grant 2014-2017 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 Letters

Issue: 2