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Table 5
Density columns (in 1022 cm-2), Gaussian EW of Fe fluorescence, abundance anomalies (solar; Fe refers to K-shell).
| Date | Binary | nHb | EW(FeK) | Fe | Ne | N |
| phase | (mÅ) | |||||
|
|
||||||
| 2001 | 0.75 | 10 | –19 | 0.10 | ~1 | ~1 |
| 2004 | 0.27 | 0.23 | –10 | 0.12 | 2.63 | 3.96 |
| 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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