The continuing formation of early-type galaxies: an H I survey

Details The continuing formation of early-type galaxies: an H I survey The continuing formation of early-type galaxies: an H I survey

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1035..129m&link_type=abstract

THE EVOLUTION OF GALAXIES THROUGH THE NEUTRAL HYDROGEN WINDOW. AIP Conference Proceedings, Volume 1035, pp. 129-131 (2008).

Computer Science

1

Cosmology, Interstellar Medium And Nebulae In External Galaxies, Galaxy Clusters, Radio Telescopes And Instrumentation, Heterodyne Receivers, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Spectroscopy And Spectrophotometry, Hi Regions And 21-Cm Lines, Diffuse, Translucent, And High-Velocity Clouds

Scientific paper

A deep H I survey of nearby early-type galaxies carried out with the Westerbork Radio Synthesis Telescope has shown that, contrary to expectation, neutral hydrogen is a significant constituent of the ISM in this type of objects located in low density environment. The studied galaxies are part of a representative sample of nearby E and SO for which integral-field spectroscopy using the SAURON spectrograph is available. We present preliminary results on the comparison of the characteristics of the H I with those of the molecular and ionised gas as well as the stellar dynamics and population.

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