Bimodality of [a Fe]-[Fe/H] distributions is a natural outcome of dissipative collapse and disc growth in Milky Way-type galaxies (2021)
Attributed to:
Astronomy Observation and Theory Consolidated Grant 2016-2019
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa3996
Publication URI: http://dx.doi.org/10.1093/mnras/staa3996
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 4