A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations * (2018)
Attributed to:
Warwick Astronomy and Astrophysics Consolidated Grant 2017-2020
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