The many reasons that the rotation curves of low-mass galaxies can fail as tracers of their matter distributions (2023)
Attributed to:
Astronomy at Durham 2020-2023
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2301.05242
Publication URI: https://arxiv.org/abs/2301.05242
Type: Other