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astro-ph1996
Observability of Early Evolutionary Phases of Galaxies at mm Wavelengths
G. De Zotti, P. Mazzei, A. Franceschini +1
Several lines of evidence and theoretical arguments suggest that a large fraction of starlight is absorbed by interstellar dust and re-radiated at far-IR wavelengths, particularly…
astro-ph1996★ 32 cited
Dust Enshrouded AGN Models for Hyperluminous High Redshift IR Galaxies
Gian Luigi Granato, Luigi Danese, Alberto Franceschini
We investigate models for the power supply and broad-band spectral energy distribution (SED) of hyperluminous IR galaxies, recently discovered at high redshifts, in terms of the em…