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Table 3.
XMM-Newton/RGS best-fit values for the isothermal cie model.
| nenHV | Temperature | O/H | Ne/H | Mg/H |
|---|---|---|---|---|
| 6.70 ± 0.08 | 4.27 |
0.47 ± 0.09 | 0.51 ± 0.09 | 0.37 ± 0.13 |
| Si/H | Fe/H | vrms | z | Cstat/d.o.f. |
| 0.31 ± 0.12 | 0.49 |
710 ± 170 | 0.2336 ± 0.0005 | 419/398 |
Notes. Abundances are in proto-Solar units (Lodders & Palme 2009), emission measure nenHV in 1073 m−3, temperature in keV and micro-turbulence 1D velocity in km s−1 (in this case representing the total width, i.e., spatial plus turbulent broadening).
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