Abstract
We present hydrodynamical simulations of galaxy clusters and groups aimed at investigating whether and how the problem of gas overcooling within galaxy clusters can be prevented by a suitable extra heating of the ICM recovering the observed X-ray scaling relations.
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References
Arnaud, M. and Evrard, A.E.: 1999, MNRAS 305, 631.
Balogh, M.L., Pearce, F.R., Bower, R.G. and Kay, S.T.: 2001, MNRAS 326, 1228.
Borgani, S., Governato, F., Wadsley, J. et al.: 2002, MNRAS, in press (preprint astro-ph/0205471).
Evrard, A.E. and Henry, J.P.: 1991, ApJ 383, 95.
Finoguenov, A., Reiprich, T.H. and Böhringer, H.: 2001, A&A 369, 479.
Kaiser, N.: 1986, MNRAS 222, 323.
Katz, N., Hernquist, L. and Weinberg, D.H.: 1992, ApJS 105, 19.
Menci, N. and Cavaliere, A.: 2000, MNRAS 311, 50.
Pearce, F.R., Thomas, P.A., Couchman, H.M.P. and Edge, A.C.: 2000, MNRAS 317, 1029.
Ponman, T.J., Bourner, P.D.J., Ebeling, H. and Böhringer, H.: 1996, 293, 690.
Ponman, T.J., Cannon, D.B. and Navarro, J.F.: 1999, Nature 397, 135.
Springel, V., Yoshida, N. and White, S.D.M.: 2001, NewA 6, 79.
Tozzi, P. and Norman, C.: 2001, ApJ 546, 63 (TN01).
Voit, G.M., Bryan, G.L., Balogh, M.L. and Bower, R.G.: 2002, ApJ, in press (preprint astroph/0205240).