Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-09T05:55:23.109Z Has data issue: false hasContentIssue false
  • English
  • Français

The Detection of CO in M104

Published online by Cambridge University Press:  03 August 2017

E. Bajaja ,
M. Krause ,
R.-J. Dettmar  and
R. Wielebinski
E. Bajaja
Affiliation:
Instituto Argentino de Radioastronomia, Casilla de Correo 5, 1894 Villa Elisa, Argentina
M. Krause
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-5300 Bonn 1, Federal Republic of Germany
R.-J. Dettmar
Affiliation:
Radioastronomisches Institut der Universität, Auf dem Hügel 71, 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

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 the early-type galaxy M104 (NGC 4594, Sombrero Galaxy) in the 12CO(1-0) transition with the 30-m IRAM telescope. We have detected CO in two positions which coincide with maxima of HI, dust and radio continuum. We failed to detect CO in the nuclear area of M104.

Type
II- Early-type and Irregular Galaxies
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 47
Copyright
Copyright © Kluwer 1991 

References

Bajaja, E. et al.: 1984, Astron. Astrophys. 141, 309 Google Scholar
Bajaja, E. et al.: 1988, Astron. Astrophys. 202, 35 Google Scholar
Thronson, H.A. Jr. et al.: 1989, Astrophys. J. 344, 747 Google Scholar
Wiklind, T., Henkel, C.: 1989, Astron. Astrophys. 225, 1 Google Scholar
Young, J.S.: 1988, in Molecular Clouds in the Milky Way and External Galaxies, eds. Dickman, R.L. et al., Springer, p. 326 Google Scholar
Young, J.S., Scoville, N.: 1982, Astrophys. J. 258, 467 CrossRefGoogle Scholar