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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

CM Baugh

CG Lacey

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