Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-09T15:28:44.675Z Has data issue: false hasContentIssue false
  • English
  • Français

The FCRAO Extragalactic CO Survey

Published online by Cambridge University Press:  03 August 2017

J.S. Young ,
L.E. Allen ,
N.A. Devereux ,
P.M. Knezek  and
S. Xie
J.S. Young
Affiliation:
Department of Physics and Astronomy and Five College Radio Astronomy Observatory University of Massachusetts, Amherst MA 01003 USA
L.E. Allen
Affiliation:
Department of Physics and Astronomy and Five College Radio Astronomy Observatory University of Massachusetts, Amherst MA 01003 USA
N.A. Devereux
Affiliation:
Department of Physics and Astronomy and Five College Radio Astronomy Observatory University of Massachusetts, Amherst MA 01003 USA
P.M. Knezek
Affiliation:
Department of Physics and Astronomy and Five College Radio Astronomy Observatory University of Massachusetts, Amherst MA 01003 USA
S. Xie
Affiliation:
Department of Physics and Astronomy and Five College Radio Astronomy Observatory University of Massachusetts, Amherst MA 01003 USA

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have observed CO J=1−0 emission in 300 galaxies at 45″ resolution as part of the FCRAO Extragalactic CO Survey. The target galaxies were selected on the basis of their optical and infrared properties, such that they are either brighter than 12th magnitude in the blue, or brighter than 10 Jy at 100 μm. This data set has been used to investigate the global ratio of molecular to atomic gas mass, the fraction of galaxy mass in neutral gas, and the yield of high mass stars per unit mass of molecular gas, all as a function of morphological type and environment.

Type
V- CO in Galactic Disks
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 148 - 150
Copyright
Copyright © Kluwer 1991 

References

Bloemen, J.B.G.L. 1986, Astr.Ap., 154, 25.Google Scholar
Devereux, N. and Young, J.S. 1990a, Ap.J.(Letters), 350, L25.Google Scholar
Devereux, N. and Young, J.S. 1990b, Ap.J., in press (Aug. 10).Google Scholar
Rengarajan, T.N. and Verma, R.P. 1987, in IAU No. 115 Star Forming Regions (eds. Peimbert, M. and Jugaku, J.).Google Scholar
Young, J.S. 1990, in the Second Wyoming Conference on the ISM in Galaxies (eds. Shull, M. and Thronson, H.).Google Scholar
Young, J.S. and Knezek, P.M. 1989, Ap.J.(Letters), 347, L55.Google Scholar
Young, J.S., Xie, S., Kenney, J., and Rice, W.L. 1989, Ap.J. Suppl., 70, 699.Google Scholar