Anatomy of the AGN in NGC 5548 - IV. The short-term variability of the outflows

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Table 3

List of the O iv and O v lines predicted by our WA model that contributes to the features visible in Fig. 5.

Ion	WA component	Outflow velocity	λ _obs ^a	τ ^b
		km s^-1	Å

O v	C	1148	20.23	27
	B	547	20.27	7
	D	254	20.29	3
	E	792	20.26	1

O iv	B	547	21.04	3
O iv	C	1148	21.00	2

O v	C	1148	22.67	143
	B	547	22.71	34
	D	254	22.73	16

O iv	C	1148	23.04	10
O iv	B	547	22.08	5

Notes.

^(a)

Predicted wavelength, considering the cosmological redshift and the blueshift due to the outflow.

^(b)

Line optical depth.

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