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Metal transport by cold fronts in M87. Aurora Simionescu (KIPAC/Stanford). METALS IN THE ICM . +. =. GAS MOTIONS IN THE ICM. Rebusco et al. 2006. Roediger et al. 2007. Simionescu et al. 2008. Markevitch&Vikhlinin 2007. Ascasibar&Markevitch 2006. Simionescu et al. in prep.
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Metal transport by cold fronts in M87 Aurora Simionescu (KIPAC/Stanford)
GAS MOTIONS IN THE ICM Rebusco et al. 2006 Roediger et al. 2007 Simionescu et al. 2008 Markevitch&Vikhlinin 2007 Ascasibar&Markevitch 2006 Simionescu et al. in prep Einstein Fellows Symposium CfA, Oct. 28, 2009 Aurora Simionescu
THE CAPPUCCINO Forman et al. 2007 Owen et al. 2000 Simionescu et al. 2008 MFe=1.5e6 Msun Einstein Fellows Symposium CfA, Oct. 28, 2009 Aurora Simionescu
THE WINE Markevitch&Vikhlinin 2007 Roediger et al. in prep Ascasibar&Markevitch 2006 Einstein Fellows Symposium CfA, Oct. 28, 2009 Aurora Simionescu
SLOSHING IN M87 courtesy of W. Forman Einstein Fellows Symposium CfA, Oct. 28, 2009 Aurora Simionescu
SLOSHING AND METAL TRANSPORT MFe=13.7e6 Msun MFe=4.5e6 Msun Simionescu et al. in prep Einstein Fellows Symposium CfA, Oct. 28, 2009 Aurora Simionescu
METAL ENRICHMENT OF ICM cD initial Leccardi et al. 2009 Einstein Fellows Symposium CfA, Oct. 28, 2009 Aurora Simionescu
METAL ENRICHMENT OF ICM Mg, O: core collapse products Fe: SN Ia product Enrichment by BCG at late times: only SN Ia -> not the only contribution to the peak Enrichment in protocluster phase much more peaked than previously thought Einstein Fellows Symposium CfA, Oct. 28, 2009 Aurora Simionescu
CONCLUSIONS & ACKNOWLEDGEMENTS • Cold fronts are very important means of broadening the metal abundance profile in the ICM • The enrichment patterns are similar close to and far away from the central cluster galaxy -> most metals produced at early times THANKS TO N. Werner, W. Forman, E. Miller, Y. Takei, H. Böhringer, E. Churazov, A. Finoguenov, P. Nulsen, E. Roediger, M. Brüggen, J. de Plaa, J. Kaastra Einstein Fellows Symposium CfA, Oct. 28, 2009 Aurora Simionescu