Star Formation in HI-Selected Galaxies

Details Star Formation in HI-Selected Galaxies Star Formation in HI-Selected Galaxies

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1035...99r&link_type=abstract

THE EVOLUTION OF GALAXIES THROUGH THE NEUTRAL HYDROGEN WINDOW. AIP Conference Proceedings, Volume 1035, pp. 99-104 (2008).

Astronomy and Astrophysics

Astronomy

Star Formation, Cosmology, Galaxy Clusters, Astronomical And Space-Research Instrumentation, Stellar Content And Populations, Radii, Morphology And Overall Structure

Scientific paper

The history and timescale of the conversion of gas into stars within galaxies define their evolution through cosmic time. HI-selected surveys of galaxies in the local universe, in combination with optical and infrared observations provide important pieces of information on the gaseous, stellar, and star-forming properties of galaxies. I present here an overview of some of the past, current and future work on stars and star-formation in HI-selected systems.

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