Molecular gas content of galaxies in the Hydra-Centaurus supercluster

Details Molecular gas content of galaxies in the Hydra-Centaurus supercluster Molecular gas content of galaxies in the Hydra-Centaurus supercluster

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993egte.conf..205h&link_type=abstract

In NASA. Ames Research Center, The Evolution of Galaxies and Their Environment p 207-208 (SEE N93-26706 10-90)

Astronomy and Astrophysics

Astronomy

Galactic Clusters, Molecular Gases, Sky Surveys (Astronomy), Spiral Galaxies, Virgo Galactic Cluster, Gas Temperature, Rotational Spectra, Submillimeter Waves, Telescopes

Scientific paper

A survey of bright spiral galaxies in the Hydra-Centaurus supercluster for the CO(1-0) transition at 115 GHz was performed with the 15m Swedish-ESO submillimeter telescope (SEST). A total of 30 galaxies have been detected in the CO(1-0) transition out of 47 observed, which is a detection rate over 60%. Global physical parameters of these galaxies derived from optical, CO, HI, and IR measurements compare very well with properties of galaxies in the Virgo cluster.

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