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

被引：0
|
作者：
Vasil'ev, EO [1 ]
机构：
[1] Rostov State Univ, Dept Phys, Rostov Na Donu 344090, Russia
来源：
OBSERVING WITH THE VLT INTERFEROMETER | 2003年 / 6卷
关键词：
D O I：
10.1051/eas:2003034
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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 Lyalpha and Halpha lines are calculated. It is shown that such PGCs can be detectable for the ongoing and future projects (VLTI, NGST).
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页码：291 / 292
页数：2
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