Density columns (in 1022 cm-2), Gaussian EW of Fe fluorescence, abundance anomalies (solar; Fe refers to K-shell).
|2010||0.74–0.96||36–74||–35 to –50||0.18||1.80||2.33|
Notes. “Fe” refers to Fe abundance from K-shell ion lines. Errors for [Fe], [N], and [Ne]: ± 0.02, ± 0.75, and ± 0.28, resp.
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