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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4438

Title: Possible forest of emission lines from protogalaxies
Authors: Nath, Biman B.
Eichler, D.
Issue Date: 1993
Publisher: Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 1993, Vol.261, pL25
Abstract: We discuss the possibility of detecting protogalaxies in the ultraviolet, assuming that galaxy formation occurred at z ~ 5-6. We show that the diffuse gas in collapsing galaxy-sized objects with temperatures ~10^6+0.5 K, and with modest metallicities, should produce many emission lines from highly ionized iron atoms. We compare the expected luminosity from models of galaxy formation with the sensitivity of the Hubble Space Telescope (HST).
Description: Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations)
URI: http://hdl.handle.net/2289/4438
ISSN: 0035-8711
1365-2966 (Online)
Alternative Location: http://adsabs.harvard.edu/abs/1993MNRAS.261L..25N
http://arxiv.org/abs/astro-ph/9301012
Copyright: 1993 Royal Astronomical Society
Appears in Collections:Research Papers (A&A)

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