Hierarchical galaxy formation

Cole, Shaun; Lacey, Cedric G.; Baugh, Carlton M.; Frenk, Carlos S.

doi:10.1046/j.1365-8711.2000.03879.x

Cited by 1,952Galaxies: Formation, Evolution, PhenomenaStellar, planetary, and galactic studiesCosmology and Gravitation Theories

Hierarchical galaxy formation

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Cole, Shaun, Lacey, Cedric G., Baugh, Carlton M., Frenk, Carlos S.·2002·Monthly Notices of the Royal Astronomical Society

DOI 10.1046/j.1365-8711.2000.03879.x

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Abstract

We describe the GALFORM semi-analytic model for calculating the formation and evolution of galaxies in hierarchical models. It improves upon, and extends, the Cole et al 1994 model. The model employs a new Monte-Carlo algorithm to follow the merging evolution of dark matter halos with arbitrary mass resolution. It incorporates realistic descriptions of the density profiles of dark matter halos and their gas content; follows the chemical evolution of gas and stars, and the associated production of dust; and includes a detailed calculation of the sizes of disks and spheroids. Wherever possible, our prescriptions for modelling individual physical processes are based on results of numerical simulations. We apply our methods to the LCDM cosmology (Omega_0=0.3, Lambda_0=0.7), and find good agreement with a wide range of properties of the local galaxy population: the B-band and K-band luminosity functions, the distribution of colours for the population as a whole, the ratio of ellipticals to spirals, the distribution of disk sizes, and the current cold gas content of disks. (Abridged)

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Cold dark matter, the structure of galactic haloes and the origin of the Hubble sequence
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A Lower Bound on the Cosmic Baryon Density
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Dynamical friction and the evolution of satellites in virialized halos: the theory of linear responsePreprint
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Formation of Disk Galaxies: Feedback and the Angular Momentum problemPreprint
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Time Evolution of Galaxy Formation and Bias in Cosmological Simulations
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Large Scale Structure: Tracks and Traces
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Authors: Cole, S., Lacey, C. G., Baugh, C. M., & Frenk, C. S.
Affiliations: Durham University (GB)
University of Copenhagen (DK)
Corresponding author: Cole, Shaun
ORCID: Lacey, Cedric G.
Baugh, Carlton M.
Frenk, Carlos S.
Venue: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Published: 2002-04-04
Volume: 319
Issue: 1
Pages: 168-204
ISSN: 0035-8711 (ISSN-L)
1365-2966
DOI: 10.1046/j.1365-8711.2000.03879.x
OpenAlex: W1929623410
Cited by: 1,952
References: 179
Citations by year: 2026: 37 · 2025: 68 · 2024: 48 · 2023: 50 · 2022: 57 · 2021: 59 · 2020: 60 · 2019: 74 · 2018: 52 · 2017: 81 · 2016: 93 · 2015: 65 · 2014: 76 · 2013: 82 · 2012: 91
FWCI: 78.89
Type: journal article
Language: en
Open access: bronze
doi.org
Locations: Monthly Notices of the Royal Astronomical Society (publishedVersion)
arXiv (Cornell University) (submittedVersion)
CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
Durham Research Online (Durham University) (submittedVersion, cc-by)
arXiv (Cornell University)
Topics: Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
Keywords: hierarchical galaxy formation, dark matter halo mergers, halo density profiles, dust formation, luminosity function, galaxy color

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