AbstractWe construct a new semi-analytic model of the evolution of dust emission of very young low-mass galaxies. We predict the contribution from forming galaxies to the fluctuation of cosmic background radiation at wavelengths of 200μm to 2.1mm. Though the contribution is very small compared with that of giant submillimeter sources at z=1–3, fluctuation signal at high-ℓ in multipole expansion (ℓ≳3×104 or θ≲20″) is unique to this forming population.
Contribution of forming galaxies to the cosmic infrared background fluctuation
Advances in Space Research ; 36 , 6 ; 1131-1135
2005-04-26
5 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Contribution of forming galaxies to the cosmic infrared background fluctuation
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