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Table 3

Parameters of the narrow absorption lines from Gaussian fits.

aλobs (Å) bλ0 (Å) Atomic transition cEW (mÅ) dv (km s-1)

15.02 Fe xvii 2p6−2p53d
18.63 O vii 1s2−1s3p 32 ± 8
18.97 O viii 1s−2p <26
22.05 O vi 1s22s−1s2s2p <24
22.35h O v 1s22s2−1s2s22p <25
23.52e 23.53 gO i <52 − 150f
23.35 gO ii f
28.47 C vi 1s−3p <35
33.74 C vi 1s−2p <31

Notes. Errors are 90% confidence intervals.

(a)

Wavelength of the line in the observer frame.

(b)

Theoretical wavelength of the line in rest frame.

(c)

Equivalent width of the line in mÅ.

(d)

Velocity of the ion in the frame of the quasar.

(e)

Line center fixed at this value.

(f)

These are velocities computed at z = 0 to represent absorption in the frame of our Galaxy.

(g)

Galatic oxygen absorption.

(h)

Theoretical value taken from Pradhan et al. (2003).

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