Abstract
AbstractWe hereafter aim to present mass estimates and main parameters of distant powerful radio sources, respectively for evolved stars, ionized gas, and dust. Observations and models are consistent with a scenario where large masses are accumulated whithin extremely short time scales < 1 Gyr at redshifts z > 2: a strong constraint for large‐scale structure models. (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
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