Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-26T03:25:28.820Z Has data issue: false hasContentIssue false
  • English
  • Français

HI Deficient Galaxies in Coma are not CO Deficient

Published online by Cambridge University Press:  03 August 2017

F. Casoli ,
F. Combes  and
P Boisse
F. Casoli
Affiliation:
Radioastronomie Millimétrique E.N.S. 24 Rue Lhomond F-5231 Paris cedex 05 France
F. Combes
Affiliation:
Radioastronomie Millimétrique E.N.S. 24 Rue Lhomond F-5231 Paris cedex 05 France
P Boisse
Affiliation:
Radioastronomie Millimétrique E.N.S. 24 Rue Lhomond F-5231 Paris cedex 05 France

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.

Spiral galaxies belonging to rich clusters are generally found to be deficient in atomic gas; this has been interpreted as being due to the ram pressure from the intracluster X-ray emitting gas or to the tidal interaction between the galaxies. However, the molecular content of spirals does not share these characteristics, at least in the Virgo cluster (Stark et al., 1986; Kenney and Young, 1989).

Type
XII- Clusters of Galaxies
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 411
Copyright
Copyright © Kluwer 1991 

References

References :

Kenney, J., Young, J.S.: 1989, Astrophys. J. 344, 171 CrossRefGoogle Scholar
Stark, A., Knapp, G., Bally, J., Wilson, R., Penzias, A., Rowe, H.: 1986, Astrophys. J. 310, 660 CrossRefGoogle Scholar