Abstract
The other members of this panel are far more knowledgable than I about galaxy evolution and the nature of the faint galaxy population. Thus, rather than address the main panel discussion topics head-on, I will instead briefly summarize some of the things we may be able to learn about the universe at high redshift from the study of two classes of objects that I know something about: AGNs at high redshift and starburst galaxies at low redshift. I will organize my remarks around several of the questions the panel has been asked to address.
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© 1993 Kluwer Academic Publishers
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Heckman, T.M. (1993). Primeval Galaxies, the IGM, and the QSO-protogalaxy Connection. In: Shull, J.M., Thronson, H.A. (eds) The Environment and Evolution of Galaxies. Astrophysics and Space Science Library, vol 188. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1882-8_11
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DOI: https://doi.org/10.1007/978-94-011-1882-8_11
Publisher Name: Springer, Dordrecht
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