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Galaxy Evolution in the Virgo Cluster

Published online by Cambridge University Press:  01 August 2006

Bernd Vollmer
Bernd Vollmer*
Affiliation:
CDS, Observatoire astronomique de Strasbourg, 11, rue de l'université, 67000 Strasbourg, France
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Abstract

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In the last years we have gained new insights on how ram pressure acts in detail on Virgo spiral galaxies. This has been possible due to the combination of new deep HI observations, deep polarized radio continuum observations, and detailed dynamical modelling (sticky particles and MHD). As a major result a first complete ram pressure stripping time sequence could be established for the Virgo cluster.

Keywords

Galaxies: clusters: individual: Virgogalaxies: interactionsgalaxies: ISMgalaxies: kinematics and dynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 155 - 159
Copyright
Copyright © International Astronomical Union 2007

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