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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S244(3), p. 378-380, 2007

DOI: 10.1017/s1743921307014366

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Tidal Influences on Cluster Dwarf Evolution

Journal article published in 2007 by R. Smith ORCID, J. I. Davies, A. Nelson
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractUsing 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.

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