The Origin of r-process Enhanced Metal-poor Halo Stars In Now-destroyed Ultra-faint Dwarf Galaxies (2019)
Attributed to:
WEAVE Detectors Interim
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aafafb
Publication URI: http://dx.doi.org/10.3847/1538-4357/aafafb
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2