All Tables

Table 1: Fit results for the RGS spectra extracted from a 1.1 $\hbox {$^\prime $ }$ wide strip centred on the core of M 87. The iron abundance is given with respect to the proto-solar values by Lodders (2003) and the other abundances with respect to iron. Emission measures ( $Y = \int n_{{\rm e}} n_{{\rm H}} {\rm d}V$ ) are given in 10⁶⁴ cm^-3.
Table 2: Fit results for spatially-resolved RGS spectra. We model the plasma with two thermal components. Abundances are given with respect to the proto-solar values by Lodders (2003). The emission measures are given in 10⁶⁴ cm^-3.
Table 3: Comparison of the observed mass ratios in the core of M 87 for five elements to iron with the predicted mass ratios, assuming that all the elements were produced only by supernovae with 86% of all iron produced by SN Ia. The observed to predicted ratio for oxygen is here by definition one.