EAS Publications Series
Volume 6, 2003Observing with the VLTI
|Page(s)||291 - 291|
|Published online||31 January 2003|
G. Perrin and F. Malbet (eds)
EAS Publications Series, 6 (2003) 291
Globular Clusters as they can be seen in Ly-alpha and H-alpha at z>1
Physics Department, Rostov State University,
Rostov on Don 344090, Russia;
Corresponding author: firstname.lastname@example.org
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 Lyα and Hα lines are calculated. It is shown that such PGCs can be detectable for the ongoing and future projects (VLTI, NGST).
© EAS, EDP Sciences, 2003
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