CM Baugh
Can the faint submillimetre galaxies be explained in the cold dark matter model?
Baugh, CM; Lacey, CG; Frenk, CS; Granato, GL; Silva, L; Bressan, A; Benson, AJ; Cole, S
Authors
CG Lacey
Professor Carlos Frenk c.s.frenk@durham.ac.uk
Professor
GL Granato
L Silva
A Bressan
AJ Benson
S Cole
Citation
Baugh, C., Lacey, C., Frenk, C., Granato, G., Silva, L., Bressan, A., …Cole, S. (2005). Can the faint submillimetre galaxies be explained in the cold dark matter model?. Monthly Notices of the Royal Astronomical Society, 356(3), 1191-1200
Journal Article Type | Article |
---|---|
Publication Date | 2005-01 |
Journal | Monthly Notices of the Royal Astronomical Society: Letters |
Print ISSN | 0035-8711 |
Publisher | Royal Astronomical Society |
Volume | 356 |
Issue | 3 |
Pages | 1191-1200 |
Keywords | galaxies : evolution; galaxies : formation; galaxies : high-redshift; submillimetreINITIAL MASS FUNCTION; ULTRAVIOLET LUMINOSITY DENSITY; SPECTRAL ENERGY-DISTRIBUTION; LYMAN-BREAK GALAXIES; STAR-FORMATION; ELLIPTIC GALAXIES; HIGH-REDSHIFT; STARBURST GALAX |
Public URL | https://durham-repository.worktribe.com/output/1564240 |
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