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- W2116530878 abstract "We describe a semi-analytic model for the X-ray emitting gas in clusters and groups in which the gas is preheated before halo formation. The model relies on physically sound prescriptions for the formation and evolution of halo structure. For a gas temperature gradient corresponding to a polytropic index of 1.2 and an energy injection of 0.6 keV per gas particle, this model successfully reproduces the observed correlations between gas luminosity, gas temperature and halo mass. We use the model to investigate the detailed entropy structure of groups and clusters of galaxies and compare the results with the observational data.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html" @default.
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- W2116530878 date "2004-03-01" @default.
- W2116530878 modified "2023-09-26" @default.
- W2116530878 title "Reproducing the entropy structure of clusters and groups" @default.
- W2116530878 doi "https://doi.org/10.1017/s1743921304000651" @default.
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