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Modeling DM and ICM in simulated galaxy clusters

Published online by Cambridge University Press:  06 October 2004

E. Rasia ,
G. Tormen  and
L. Moscardini
E. Rasia
Affiliation:
Dipartimento di Astronomia, Università di Padova, vicolo dell'Osservatorio 2, I-3512, Padova, Italy email: rasia@pd.astro.it
G. Tormen
Affiliation:
Dipartimento di Astronomia, Università di Padova, vicolo dell'Osservatorio 2, I-3512, Padova, Italy email: rasia@pd.astro.it
L. Moscardini
Affiliation:
Dipartimento di Astronomia, Università di Bologna, via Ranzani 1, I-40127, Bologna, Italy
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Abstract

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Using the results of an extended set of high-resolution non-radiative hydrodynamic simulations of galaxy clusters we obtain simple analytic formulae for the dark matter and hot gas distribution, in the spherical approximation.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUC195 , March 2004 , pp. 309 - 312
Copyright
© 2004 International Astronomical Union