Molecular Gas and Star Formation in Luminous IR Galaxies and QSO Hosts

Details Molecular Gas and Star Formation in Luminous IR Galaxies and QSO Hosts Molecular Gas and Star Formation in Luminous IR Galaxies and QSO Hosts

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..395..113e&link_type=abstract

Frontiers of Astrophysics: A Celebration of NRAO's 50th Anniversary ASP Conference Series, Vol. 395, Proceedings of the conferen

Astronomy and Astrophysics

Astrophysics

Scientific paper

Millimeter and radio-wave facilities built and operated by the NRAO have played a major role in increasing our understanding of the interstellar medium and radio continuum properties of luminous IR galaxy (LIRG) mergers and quasi-stellar object (QSO) hosts. This review focuses primarily on molecular gas (CO) surveys of the local (z<0.3) population of both galaxy classes and the relevance of these observations to their star-formation properties.

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