Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-02-03
Mon.Not.Roy.Astron.Soc. 323 (2001) 67
Astronomy and Astrophysics
Astrophysics
9 pages, 6 figures. Accepted for publication in MNRAS Introduction ammended, figure added, references added
Scientific paper
10.1046/j.1365-8711.2001.04091.x
Observations in the submillimetre waveband have recently revealed a new population of luminous, sub-mm sources. These are proposed to lie at high redshift and to be optically faint due to their high intrinsic dust obscuration. The presence of dust has been previously invoked in optical galaxy count models which assume $\tau=9$ Gyr Bruzual & Charlot evolution for spirals and these fit the count data well from U to K. We now show that by using either a 1/$\lambda$ or Calzetti absorption law for the dust and re-distributing the evolved spiral galaxy UV radiation into the far infra-red(FIR), these models can account for all of the `faint'($\leq1$mJy) $850\mu$m galaxy counts, but fail to fit 'bright'($\ge2$mJy) sources, indicating that another explanation for the sub-mm counts may apply at brighter fluxes(e.g. QSOs, ULIRGs). We find that the main contribution to the faint, sub-mm number counts is in the redshift range $0.5 < z < 3$, peaking at $z\approx 1.8$. The above model, using either dust law, can also explain a significant proportion of the extra-galactic background at $850\mu$m as well as producing a reasonable fit to the bright $60\mu m$ IRAS counts.
Busswell Geoff S.
Shanks Tom
No associations
LandOfFree
The Contribution of Faint Blue Galaxies to the Sub-mm Counts and Background does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Contribution of Faint Blue Galaxies to the Sub-mm Counts and Background, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Contribution of Faint Blue Galaxies to the Sub-mm Counts and Background will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-390765