I review the insights emerging from recent large kinematic surveys of galaxies at low redshift, with particular reference to the SAMI, CALIFA and MaNGA surveys. These new observations provide a more comprehensive picture of the angular momentum properties of galaxies over wide ranges in mass, morphology and environment in the present-day universe. I focus on the distribution of angular momentum within galaxies of various types and the relationship between mass, morphology and specific angular momentum. I discuss the implications of the new results for models of galaxy assembly.
@article{arxiv.1811.01518,
title = {Emerging angular momentum physics from kinematic surveys},
author = {Matthew Colless},
journal= {arXiv preprint arXiv:1811.01518},
year = {2020}
}
Comments
To appear in 'Galactic Angular Momentum', edited by Danail Obreschkow, the proceedings of Focus Meeting 6 held during the XXXth IAU General Assembly, August 2018 (6 pages, 7 figures). arXiv admin note: text overlap with arXiv:1608.00291