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Recombination emission from protoglobular clouds on high redshifts
Authors:EO Vasiliev  YuA Shchekinov
Institution:(1) Physics Department, Rostov State University, Rostov on Don, Russia, 344090
Abstract:Fluxes in hydrogen and helium lines from Proto-Globular Clusters (PGCs) at redshifts z > 1 are estimated. A supernovae remnant in PGCs is considered as a possible source. Intensities in Lyα,Hα and 1640 Å HeI are calculated. It is shown that such PGCs can be detectable for the ongoing and future projects.
Keywords:early-type galaxy  globular cluster  supernovae
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