Table 2: Strongest RGS lines of MP Mus.
\begin{displaymath}{ \begin{tabular}{rrlcr@{$~\pm~$}l} \hline\hline\noalign{\sma... ...sc vi} C {\sc vi} & 6.10 & 16.4 & 5.2 \\ \hline \end{tabular}}\end{displaymath}
a Observed and predicted (APED database) wavelengths (Å). b Temperature (K) of maximum emissivity. c Line fluxes ( ${\rm 10^{-6}~ph~s^{-1}~cm^{-2}}$) with uncertainties at the 68% confidence level.

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