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Tidal Influences on Cluster Dwarf Evolution

Published online by Cambridge University Press:  01 June 2007

R. Smith ,
J. I. Davies  and
A. Nelson
R. Smith
Affiliation:
School of Physics & Astronomy, University of Wales, Cardiff, UK
J. I. Davies
Affiliation:
School of Physics & Astronomy, University of Wales, Cardiff, UK
A. Nelson
Affiliation:
School of Physics & Astronomy, University of Wales, Cardiff, UK
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Abstract

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Using N-Body/Treecode, SPH simulations, including a self regulating Star Formation-feedback model, the influence of cluster tidal forces on infalling dwarf irregulars is investigated. Results suggest that an encounter with the cluster potential can disrupt a rotating disk causing morphological transformation of the gaseous component, resulting in an enhancement of star formation rates (SFRs) of up to an order of magnitude.

Information

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S244: Dark Galaxies and Lost Baryons , June 2007 , pp. 378 - 380
Copyright
Copyright © International Astronomical Union 2008

References

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