Preprint
How to bend galaxy disc profiles: the role of halo spin
Abstract
The radial density profiles of stellar galaxy discs can be well approximated
as an exponential. Compared to this canonical form, however, the profiles in
Authors
Herpich J; Stinson GS; Dutton AA; Rix H-W; Martig M; Roškar R; Macciò AV; Quinn TR; Wadsley J
Publication date
January 8, 2015
DOI
10.48550/arxiv.1501.01960
Preprint server
arXiv