Report on the Workshop Multiwavelength Views of the ISM in High-redshift Galaxies

Details Report on the Workshop Multiwavelength Views of the ISM in High-redshift Galaxies Report on the Workshop Multiwavelength Views of the ISM in High-redshift Galaxies

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011msngr.145...46w&link_type=abstract

The Messenger, vol. 145, p. 46-48

Physics

Scientific paper

Our knowledge of the formation and evolution of distant galaxies continues to advance dramatically with the advent of new facilities at most observable wavelengths. One of the outstanding questions related to this field is: How do galaxies get their gas? Over the next decade, radio and submillimetre facilities like the Expanded Very Large Array and the Atacama Large Millimeter/submillimeter Array will probe the chemistry, kinematics and obscured star formation properties of the interstellar medium in galaxies at high redshift, allowing this question to be addressed. We report on a timely workshop on the roles of theory and multi-wavelength observing facilities in furthering our understanding of interstellar medium physics in distant galaxies.

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