HI 21 cm Absorption Studies: Prospects

Details HI 21 cm Absorption Studies: Prospects HI 21 cm Absorption Studies: Prospects

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1035...57k&link_type=abstract

THE EVOLUTION OF GALAXIES THROUGH THE NEUTRAL HYDROGEN WINDOW. AIP Conference Proceedings, Volume 1035, pp. 57-62 (2008).

Astronomy and Astrophysics

Astronomy

Origin And Formation Of The Universe, Galaxy Clusters, Interstellar Medium And Nebulae In External Galaxies, Astronomical And Space-Research Instrumentation, Origin, Formation, Evolution, Age, And Star Formation, Star Formation

Scientific paper

HI 21 cm absorption spectroscopy of damped Lyman-α systems (DLAs) towards radio-loud background sources provides an interesting probe of the nature of the absorbing galaxies, yielding information on their ISM conditions, kinematics and spatial extent. In this article, I will describe our recent results from such HI 21 cm absorption studies, before discussing prospects for the field with upcoming instruments like ASKAP and the EVLA.

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