The evolution of the stellar mass versus halo mass relationship

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 23 Dec 2015Embargo end date: 01 Jan 2015 English Publisher:Oxford University Press (OUP)Journal:Monthly Notices of the Royal Astronomical Society, volume 456, pages 1,459-1,483 (issn: 0035-8711, eissn: 1365-2966,

Copyright policy )Funded by:UKRI | The Virgo consortium for ..., UKRI | Durham DiRAC-2 petascale ..., UKRI | Quota Studentship 2011 +1 projects

Authors: Mitchell, Peter D.; Lacey, Cedric G.; Baugh, Carlton M.; Cole, Shaun;

doi: 10.1093/mnras/stv2741 , 10.48550/arxiv.1510.08463

arXiv: 1510.08463

The evolution of the stellar mass versus halo mass relationship

- Summary
- Subjects
- Metrics

Abstract

We present an analysis of the predictions made by the Galform semi-analytic galaxy formation model for the evolution of the relationship between stellar mass and halo mass. We show that for the standard implementations of supernova feedback and gas reincorporation used in semi-analytic models, this relationship is predicted to evolve weakly over the redshift range 0

Submitted to MNRAS after first round of referee comments, 26 pages, 16 figures, fixed a reference

Related Organizations

Durham University
United Kingdom
Durham University

Keywords

haloes [Galaxies], Galaxies: evolution, FOS: Physical sciences, Galaxies: formation, stellar content. [Galaxies], Galaxies: stellar content, evolution [Galaxies], formation [Galaxies], Astrophysics - Astrophysics of Galaxies, 520, Astrophysics of Galaxies (astro-ph.GA), Galaxies: haloes

Impact byBIP!

	selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	40
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Top 10%
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Average
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Top 10%