Journal Article

The coevolution of the velocity and mass functions of galaxies and dark haloes

Kyu-Hyun Chae

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 413, issue 2, pages 887-900
Published in print May 2011 | ISSN: 0035-8711
Published online April 2011 | e-ISSN: 1365-2966 | DOI:
The coevolution of the velocity and mass functions of galaxies and dark haloes

More Like This

Show all results sharing this subject:

  • Astronomy and Astrophysics


Show Summary Details


We employ a bias-corrected abundance-matching technique to investigate the coevolution of the Lambda cold dark matter (ΛCDM) dark halo mass function (HMF), the observationally derived velocity dispersion and stellar mass functions (VDF, SMF) of galaxies between z= 1 and 0. We use for the first time the evolution of the VDF constrained through strong lensing statistics by Chae for galaxy–halo abundance-matching studies. As a local benchmark we use a couple of z∼ 0 VDFs [a Monte Carlo realized VDF based on Sloan Digital Sky Survey (SDSS) Data Release 5 (DR5) and a directly measured VDF based on SDSS DR6]. We then focus on connecting the VDF evolution to the HMF evolution predicted by N-body simulations and the SMF evolution constrained by galaxy surveys. On the VDF–HMF connection, we find that the local dark halo virial mass–central stellar velocity dispersion (Mvir–σ) relation is in good agreement with the individual properties of well-studied low-redshift dark haloes, and the VDF evolution closely parallels the HMF evolution meaning little evolution in the Mvir–σ relation. On the VDF–SMF connection, it is also likely that the stellar mass–stellar velocity dispersion (M–σ) relation evolves little, taking the abundance-matching results together with other independent observational results and hydrodynamic simulation results. Our results support the simple picture that as the halo grows hierarchically, the stellar mass and the central stellar velocity dispersion grow in parallel. We discuss possible implications of this parallel coevolution for galaxy formation and evolution under the ΛCDM paradigm.

Keywords: galaxies: evolution; galaxies: formation; galaxies: haloes; galaxies: kinematics and dynamics; galaxies: statistics; galaxies: structure

Journal Article.  12704 words.  Illustrated.

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.