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CO Observations of Southern Galaxies

Published online by Cambridge University Press:  03 August 2017

E. Bajaja ,
H.-P. Reuter ,
R. Wielebinski ,
J.I. Harnett  and
E. Hummel
E. Bajaja
Affiliation:
Instituto Argentino de Radioastronomia, Casilla de Correo 5, 1894 Villa Elisa, Argentina
H.-P. Reuter
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-5300 Bonn 1, Federal Republic of Germany
R. Wielebinski
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-5300 Bonn 1, Federal Republic of Germany
J.I. Harnett
Affiliation:
School of Physics, University of Sydney, Sydney NSW 2006, Australiann 1, Federal Republic of Germany
E. Hummel
Affiliation:
Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, United Kingdom

Extract

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We have mapped the southern galaxies NGC 613, 1313, 1433, 1566, 1672, and 2442 in the 12CO(1-0) line with the SEST telescope. The sample bases on galaxies observed previously in radio continuum at the Molonglo Observatory (Harnett, 1985).

Type
V- CO in Galactic Disks
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 159
Copyright
Copyright © Kluwer 1991 

References

Bajaja, E., Hummel, E.: 1989, ESO Messenger 55, 37 Google Scholar
Buta, R.: 1986, Astrophys. J. Suppl. 61, 631 CrossRefGoogle Scholar
Harnett, J.I.: 1985, Ph.D. Thesis, University of Sydney Google Scholar
Sersic, J.L., Calderon, J.H.: 1979, Astrophys. Space Sci. 62, 211 CrossRefGoogle Scholar