All Tables

Table 1: XMM-Newton GTO observations of RX J0852.0-4622.
Table 2: Spectral fit results with a wabs(vmekal)+wabs(vmekal+power law) model for the range $0.2\leq E_{\rm x} \leq 10$ keV.
Table 3: Fit results for $E_{\rm x}\geq 0.8$ keV with various spectral models for the continuum including a power law, the sresc model with and without one or two Gaussian lines.
Table 4: Line feature parameters derived from the XMM spectra of the SNR rims.
Table 5: Positions, relative intensities of lines and K-shell fluorescent yields of the abundant elements expected for the SNR RX J0852.0-4622 outer shell.