Recombination emission from protoglobular clouds on high redshifts

Details Recombination emission from protoglobular clouds on high redshifts Recombination emission from protoglobular clouds on high redshifts

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.284..365v&link_type=abstract

Astrophysics and Space Science, v. 284, Issue 2, p. 365-368 (2003).

Astronomy and Astrophysics

Astrophysics

Early-Type Galaxy, Globular Cluster, Supernovae

Scientific paper

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.

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