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The distribution of mass components in simulated...
Preprint

The distribution of mass components in simulated disc galaxies

Abstract

Using 22 hydrodynamical simulated galaxies in a LCDM cosmological context we recover not only the observed baryonic Tully-Fisher relation, but also the

Authors

Santos-Santos IM; Brook CB; Stinson G; Di Cintio A; Wadsley J; Domínguez-Tenreiro R; Gottlöber S; Yepes G

Publication date

October 8, 2015

DOI

10.48550/arxiv.1510.02474

Preprint server

arXiv