EAS Publications Series

Issue		EAS Publications Series Volume 6, 2003 Observing with the VLTI
Page(s)		291
DOI		10.1051/eas:2003034

Observing with the VLTI
G. Perrin and F. Malbet (eds)
EAS Publications Series, Vol. 6, 2003
DOI: 10.1051/eas:2003034

Globular Clusters as they can be seen in Ly-alpha and H-alpha at z>1

E.O. Vasil'ev

Physics Department, Rostov State University, Rostov on Don 344090, Russia;

eustarru@mail.yahoo.co.uk

Abstract
Fluxes in Ly-alpha and H-alpha lines from Proto Globular Clusters (PGCs) at redshifts z>1 are estimated. Two possible sources are considered: HII regions and supernovae remnats in PGCs. Intensities in Ly $\alpha$ and H $\alpha$ lines are calculated. It is shown that such PGCs can be detectable for the ongoing and future projects (VLTI, NGST).

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