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The Evolution of the Tully-Fisher Relation: Characterizing the Assembly of Rotation-Dominated Disk Galaxies over cosmic time

Published onMay 31, 2019
The Evolution of the Tully-Fisher Relation: Characterizing the Assembly of Rotation-Dominated Disk Galaxies over cosmic time
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Abstract

We describe how to examine the properties of rotation-dominated (RD) disk galaxies over cosmic time by probing a large range in mass and luminosity, down to the sub-L* population. The science goal is to characterize the evolution of RD disk galaxies. This white paper pertains to the “Galaxy evolution” panel of the Astro2020 Decadal Survey.

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