The many reasons that the rotation curves of low-mass galaxies can fail as tracers of their matter distributions (2023)

First Author: Downing E

Attributed to: DiRAC 2.5y Bridging Funding - UCL funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stad868

Publication URI: http://dx.doi.org/10.1093/mnras/stad868

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 3