Till Sawala
The chosen few: the low-mass haloes that host faint galaxies
Sawala, Till; Frenk, Carlos S.; Fattahi, Azadeh; Navarro, Julio F.; Theuns, Tom; Bower, Richard G.; Crain, Robert A.; Furlong, Michelle; Jenkins, Adrian; Schaller, Matthieu; Schaye, Joop
Authors
Professor Carlos Frenk c.s.frenk@durham.ac.uk
Professor
Azadeh Fattahi
Julio F. Navarro
Professor Tom Theuns tom.theuns@durham.ac.uk
Professor
Richard G. Bower
Robert A. Crain
Michelle Furlong
Professor Adrian Jenkins a.r.jenkins@durham.ac.uk
Professor
Matthieu Schaller
Joop Schaye
Abstract
Since reionization prevents star formation in most haloes less massive than 3 × 109 M⊙, dwarf galaxies only populate a fraction of existing dark matter haloes. We use hydrodynamic cosmological simulations of the Local Group to study the discriminating factors for galaxy formation in the early Universe and connect them to the present-day properties of galaxies and haloes. A combination of selection effects related to reionization, and the subsequent evolution of haloes in different environments, introduces strong biases between the population of haloes that host dwarf galaxies, and the total halo population. Haloes that host galaxies formed earlier and are more concentrated. In addition, haloes more affected by tidal stripping are more likely to host a galaxy for a given mass or maximum circular velocity, vmax, today. Consequently, satellite haloes are populated more frequently than field haloes, and satellite haloes of 108–109 M⊙ or vmax of 12–20 km s−1, compatible with stellar kinematics of Local Group dwarf spheroidals, have experienced a greater than average reduction in both mass and vmax after infall. They are on closer, more radial orbits with higher infall velocities and earlier infall times. Together, these effects make dwarf galaxies highly biased tracers of the underlying dark matter distribution.
Citation
Sawala, T., Frenk, C. S., Fattahi, A., Navarro, J. F., Theuns, T., Bower, R. G., …Schaye, J. (2016). The chosen few: the low-mass haloes that host faint galaxies. Monthly Notices of the Royal Astronomical Society, 456(1), 85-97. https://doi.org/10.1093/mnras/stv2597
Journal Article Type | Article |
---|---|
Acceptance Date | Nov 3, 2015 |
Online Publication Date | Dec 11, 2015 |
Publication Date | Feb 11, 2016 |
Deposit Date | Feb 19, 2016 |
Publicly Available Date | Feb 23, 2016 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 456 |
Issue | 1 |
Pages | 85-97 |
DOI | https://doi.org/10.1093/mnras/stv2597 |
Keywords | Methods: numerical, Galaxies: dwarf, Galaxies: formation, Local Group, Cosmology: theory. |
Public URL | https://durham-repository.worktribe.com/output/1411686 |
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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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