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Star Formation Through Cosmic Time

Published online by Cambridge University Press:  01 August 2006

Michael A. Dopita
Michael A. Dopita*
Affiliation:
Research School of Astronomy & Astrophysics, Australian National University, Mt. Stromlo Observatory, Cotter Road, Weston Creek, ACT 2611, Australia email: [email protected]
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Abstract

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This paper reviews the star formation history of the Universe, from the first stars to the current day, with emphasis on the critical analysis of the techniques that have been used to determine it, especially considering the role of dust. We consider the first population of stars, the Population III stars, were formed at redshifts ranging as high as z ~ 60, the formation of the Globular Clusters, the main epoch of galaxy formation. In the sub-mm galaxies and high-redshift radio galaxies the collapse of massive galaxies was surprisingly rapid, and that the growth of super-massive black holes at their centers provides the energy input to eject the galactic interstellar medium while at the same time precipitating a final burst of star formation and the ejection of their ISM so that the subsequent evolution of these galaxies is passive.

Keywords

Physical Processes: neutrinosshock wavesISM: dustHII regionsGalaxies: formationevolutionhigh-redshiftjets
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 261 - 267
Copyright
Copyright © International Astronomical Union 2007

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