Professor Cedric Lacey cedric.lacey@durham.ac.uk
Professor
Tidally triggered galaxy formation. I - Evolution of the galaxy luminosity function
Lacey, Cedric; Silk, Joseph
Authors
Joseph Silk
Abstract
Motivated by accumulating evidence that large-scale galactic star formation is initiated and sustained by tidal interactions, a phenomenological model is developed for the galaxy luminosity function, commencing from a galaxy mass function that is predicted by a hierarchical model of structure formation such as the cold dark matter dominated cosmology. The epoch of luminous galaxy formation and the galactic star-formation rate are determined by the environment. Gas cooling and star-formation feedback are incorporated; the present epoch luminosity function of bright galaxies and the distribution of galaxy colors are well reproduced. Biasing, via the preferential formation of luminous galaxies in denser regions associated with groups of clusters, is a natural outcome of this tidally triggered star-formation model. A large frequency is inferred of 'failed' galaxies, prematurely stripped by supernova-driven winds, that populate groups and clusters in the form of low surface brightness gas-poor dwarfs, and of 'retarded' galaxies, below the threshold for effective star formation, in the field, detectable as gas-rich, extremely low surface brightness objects. Predictions are presented for the evolution with redshift of the distribution of characteristic star formation timescales, galaxy ages, and colors. Estimates are also made of galaxy number counts, and it is suggested that dwarf galaxies undergoing bursts of star formation at z of about 1 may dominate the counts at the faintest magnitudes.
Citation
Lacey, C., & Silk, J. (1991). Tidally triggered galaxy formation. I - Evolution of the galaxy luminosity function. Astrophysical Journal, 381, 14-32. https://doi.org/10.1086/170625
Journal Article Type | Article |
---|---|
Publication Date | Nov 1, 1991 |
Deposit Date | Feb 16, 2015 |
Publicly Available Date | Mar 20, 2015 |
Journal | Astrophysical Journal |
Print ISSN | 0004-637X |
Electronic ISSN | 1538-4357 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 381 |
Pages | 14-32 |
DOI | https://doi.org/10.1086/170625 |
Keywords | Galactic evolution, Milky Way Galaxy, Star formation, Astronomical models, Astronomical photometry, Galactic radiation, Luminosity, Tides. |
Files
Published Journal Article
(481 Kb)
PDF
Copyright Statement
© 1991. The American Astronomical Society. All rights reserved.
You might also like
The complex interplay of AGN jet-inflated bubbles and the intracluster medium
(2023)
Journal Article
Active galactic nuclei jets simulated with smoothed particle hydrodynamics
(2023)
Journal Article
QWIND3: UV line-driven accretion disc wind models for AGN feedback
(2022)
Journal Article
Spin-driven jet feedback in idealized simulations of galaxy groups and clusters
(2022)
Journal Article