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A Molecular Gas Ring in NGC 1808

Published online by Cambridge University Press:  03 August 2017

M. Dahlem
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
B. Koribalski
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-5300 Bonn 1, Federal Republic of Germany Radioastronomisches Institut der Universität, Auf dem Hügel 71, D-5300 Bonn 1, Federal Republic of Germany
U. Mebold
Affiliation:
Radioastronomisches Institut der Universität, Auf dem Hügel 71, D-5300 Bonn 1, Federal Republic of Germany

Extract

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The active galaxy NGC 1808 has been studied in 12CO(1-0) and 12CO(2-1) transitions with the SEST telescope and in HI and radio continuum with the VLA.

Type
VIII- Bars, Rings and Starbursts
Copyright
Copyright © Kluwer 1991 

References

Dahlem, M., Aalto, S., Klein, U., Booth, R., Mebold, U., Wielebinski, R., Lesch, H.: 1990, Astron. Astrophys. (in press) Google Scholar
Loiseau, N., Nakai, N., Sofue, Y., Wielebinski, R., Reuter, H.-P., Klein, U.: 1990, Astron. Astrophys. 228, 331 Google Scholar
Saikia, D.J., Unger, S.W., Pedlar, A., Yates, G.J., Axon, D.J., Wolstencroft, R.D., Taylor, K., Gyldenkerne, K.: 1990, Monthly Notices Roy. Astron. Soc. (in press) Google Scholar