Open AccessModelling SCUBA sources in a ΛCDM cosmology: hot starbursts or cold extended galactic dust?
Author(s) -
Kaviani A.,
Haehnelt M. G.,
Kauffmann G.
Publication year - 2003
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2003.06318.x
Subject(s) - physics , astrophysics , spectral energy distribution , galaxy , redshift , star formation , flux (metallurgy) , luminous infrared galaxy , astronomy , optical depth , cosmology , active galactic nucleus , materials science , aerosol , meteorology , metallurgy
Previous modelling has demonstrated that it is difficult to reproduce the SCUBA source counts within the framework of standard hierarchical structure formation models if the sources are assumed to be the high‐redshift counterparts of local ultraluminous infrared galaxies with dust temperatures in the range 40–60 K. Here, we show that the counts are more easily reproduced in a model in which the bulk of the submillimetre emission comes from extended, cool (20–25 K) dust in objects with star formation rates of 50–100 M ⊙ yr −1 . The low temperatures imply typical sizes of ∼1 ( S 850 /1 mJy) 1/2 arcsec , a factor of 2–3 larger than those predicted using starburst‐like spectral energy distributions. Low dust temperatures also imply a ratio of optical/ultraviolet to 850‐μm flux that is 30–100 times smaller, for the same optical depth, than expected for objects with a hot, starburst‐like spectral energy distribution. This may help to explain the small overlap between SCUBA sources and Lyman‐break galaxies.