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Galaxy evolution from cluster and absorption-selected samples

  • Part I The Universe at High-z
  • Conference paper
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The Universe at High-z, Large-Scale Structure and the Cosmic Microwave Background

Part of the book series: Lecture Notes in Physics ((LNP,volume 470))

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Abstract

Rich clusters of galaxies and QSO absorption line systems provide two alternative venues for studying the evolution of galaxies at high redshift. Here I review some recent observational results in both areas of investigation, and consider their implications for the history of galaxy evolution since z∼1.

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Enrique Martínez-González Jose Luis Sanz

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© 1996 Springer-Verlag

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Dickinson, M. (1996). Galaxy evolution from cluster and absorption-selected samples. In: Martínez-González, E., Sanz, J.L. (eds) The Universe at High-z, Large-Scale Structure and the Cosmic Microwave Background. Lecture Notes in Physics, vol 470. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0102577

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  • DOI: https://doi.org/10.1007/BFb0102577

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-61225-4

  • Online ISBN: 978-3-540-68386-5

  • eBook Packages: Springer Book Archive

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