A polar+equatorial wind model for broad absorption line quasars - I. Fitting the C IV BAL profiles

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Volume 515 (June 2010)

A&A, 515 (2010) A22

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Table 2:

Parameter of the two-component wind model for the best fit of the C IV BALs in the selected quasar sample.
BAL QSO Name	z	$\tau_{\rm tot_p}$	$k_{\rm pm}$	${v}_{\rm max}^{\rm po}$ ( $\rm {km~s}^{-1}$ )	${v}_{\rm max}^{\rm eq}$ ( $\rm {km~s}^{-1}$ )	${V}_{\rm rot}$ ( $\rm {km~s}^{-1}$ )	$\alpha$	$\beta$	$\Delta \theta$ ( $\hbox{$^\circ$ }$ )	i ( $\hbox{$^\circ$ }$ )	$f_{\rm e}$	$\gamma$
Q1333+2840	1.897	3.00	10.0	13 000	4000	1000	3.0	0.8	10	80	0.21	1.0
Q1413+1143	2.522	10.0	15.0	11 000	3500	2000	3.0	0.8	10	88	0.16	1.0
Q0145+0416	1.990	1.00	12.0	18 000	9600	6400	2.5	1.2	15	80	0.18	1.0
Q0226-1024	2.164	1.00	10.0	25 000	12500	12500	2.0	1.5	15	87	0.10	1.0
Q0321-3344	1.955	10.0	10.0	10 000	7500	5200	2.5	1.5	15	75	0.16	1.0
Q0842+3431	2.100	14.0	5.00	16 000	10000	8000	3.0	1.5	15	78	0.04	1.0
Q1235+1453	2.835	5.00	10.0	13 000	8000	7000	2.5	1.5	15	76	0.12	1.0
Q1239+0995	1.970	3.00	5.00	16 000	8000	8000	3.0	1.0	15	82	0.10	1.0
Q0019+0107 M1	2.075	1.00	15.0	16 000	9000	8000	2.5	1.5	15	90	0.11	1.0
Q0019+0107 M2	2.075	0.00	15.0^a	-	9000	8000	2.5	1.5	15	90	0.11	1.0
Q0041-4023 M1	2.450	5.00	10.0	10 000	5000	3000	2.0	1.5	15	90	0.18	1.0
Q0041-4023 M2	2.450	15.0	5.0	6000	3000	3000	2.0	0.5	15	0	0.07	1.0

Notes. ^(a) $k_{\rm pm}$ represents the total equatorial ( $i=90 \hbox {$^\circ $ }$ ) optical depth integrated over frequencies since $\tau_{\rm tot_p}=0$ .

Source LaTeX | All tables | In the text

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