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Evolution of Normal Galaxies: HST Morphologies and Deep Spectroscopy

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The Early Universe with the VLT

Part of the book series: ESO Astrophysics Symposia ((ESO))

Abstract

I review progress in understanding the evolution of normal field and cluster galaxies through the combination of HST imaging and ground-based spectroscopy. These data suggest that the bulk of the star formation producing the present-day galaxy population occurred at accessible redshifts, z < 2. Furthermore, a surprising amount of the detailed processing that shaped the Hubble sequence and morphology-density relation occurred surprisingly recently. The stage is thus set for a concerted attack on these questions with the present generation of 8–10 metre large telescopes. An important step forward will be the development of efficient survey techniques for the systematic exploration of the z >1 Universe. Some possible approaches are briefly discussed.

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© 1997 Springer-Verlag Berlin Heidelberg

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Ellis, R. (1997). Evolution of Normal Galaxies: HST Morphologies and Deep Spectroscopy. In: Bergeron, J. (eds) The Early Universe with the VLT. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-49709-7_7

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  • DOI: https://doi.org/10.1007/978-3-540-49709-7_7

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-662-22488-5

  • Online ISBN: 978-3-540-49709-7

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