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Modeling DM and ICM in simulated galaxy clusters
Published online by Cambridge University Press: 06 October 2004
Abstract
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
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