Galaxy Evolution Begins at Home: ATA-256 and Other SKA Pathfinders

Details Galaxy Evolution Begins at Home: ATA-256 and Other SKA Pathfinders Galaxy Evolution Begins at Home: ATA-256 and Other SKA Pathfinders

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21720307s&link_type=abstract

American Astronomical Society, AAS Meeting #217, #203.07; Bulletin of the American Astronomical Society, Vol. 43, 2011

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Scientific paper

While studies of galaxy evolution generally focus on extensive HI surveys at large redshifts, understanding of detailed physical processes that drive HI evolution in galaxies is equally important. Specifically, we focus on two open questions regarding the very first step in the star-formation cycle in galaxies: How much do galaxy halos flavor and tax the accretion flows that are postulated to bring fresh star-formation fuel to galaxy disks? What are the basic properties of the warm neutral gas, the progenitor of cold star-forming clouds? The very local Universe (The Milky Way and nearby galaxies) offers an unparalleled high-resolution view for answering these questions and ATA-256 and other SKA pathfinders promise great advances.

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