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Effects of environment on the properties of cluster galaxies via ram pressure stripping

Published online by Cambridge University Press:  21 October 2010

T. E. Tecce ,
S. A. Cora ,
P. B. Tissera  and
M. G. Abadi
T. E. Tecce
Affiliation:
Instituto de Astronomía y Física del Espacio, CONICET-UBA, CC 67 Suc. 28, C1428ZAA Buenos Aires, Argentina.
S. A. Cora
Affiliation:
Facultad de Ciencias Astronómicas y Geofísicas, UNLP and Instituto de Astrofísica de La Plata, CONICET, Paseo del Bosque S/N, B1900FWA La Plata, Argentina.
P. B. Tissera
Affiliation:
Instituto de Astronomía y Física del Espacio, CONICET-UBA, CC 67 Suc. 28, C1428ZAA Buenos Aires, Argentina.
M. G. Abadi
Affiliation:
Observatorio Astronómico, UNC, Laprida 854, X5000BGR Córdoba, Argentina. email: tomas@iafe.uba.ar
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Abstract

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We study the effect of ram pressure stripping (RPS) on the colours, cold gas content and star formation of galaxies in clusters, using a combination of N-Body/SPH simulations of galaxy clusters and a semi-analytic model of galaxy formation that includes the effect of RPS.

Keywords

Galaxies: clusters: generalgalaxies: evolutionintergalactic medium
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 294
Copyright
Copyright © International Astronomical Union 2010

References

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