Table 1: Atomic lines detected in the FUSE spectrum of HD 141569A. The velocities are in the pipeline's rest frame (observed spectrum) and are heliocentric. For the saturated lines, we measured the velocity of the centroid; for those lines the error bars on the velocity are symetric (not calculated by a $\chi ^2$ minimization). The radial velocities and line widths have been determined using respectively all the unsaturated and saturated lines of a given ion. "sat'' and "unsat'' are respectively for saturated and unsaturated lines. -^a line not fitted because of the very low S/N ratio of the data; -^b Doppler parameter b not measured because of the unsaturated state of the line.
Element Wavelength Energy level Line Radial velocity N b

Å (cm^-1) State (km s^-1) (cm^-2) (km s^-1)

Ar I 1048.2198 0.00 -^a - $27.0\pm3$ > $7.30\times10^{14}$ $\rm 5.6_{-0.25}^{+0.42}$

1066.6599 0.00 sat

FeII
1063.1764 0.00 unsat $\rm -24.28_{-2.75}^{+1.89}$ $\rm 9.77_{-0.94}^{+4.56}\times10^{15}$ $\rm 2.34_{-0.79}^{+0.25}$

1096.8770 0.00 sat

1121.9749 0.00 unsat

1143.2260 0.00 unsat

1144.9379 0.00 sat

FeII*
1068.3456 384.79 unsat $\rm -24.28_{-2.75}^{+1.89}$ $\rm 5.21_{-1.25}^{+3.65}\times10^{13}$ $\rm 2.34_{-0.79}^{+0.25}$

1096.6073 384.79 unsat

1147.4092 384.79 unsat

1148.2773 384.79 unsat

FeII**
1071.5842 667.68 unsat $\rm -24.28_{-2.75}^{+1.89}$ $4.25_{-2.65}^{+4.36}\times10^{13}$ $\rm 2.34_{-0.79}^{+0.25}$

1151.1458 667.68 unsat

FeII***
1148.0789 862.61 unsat -24.28 _-2.75^+1.89 $2.77_{-0.89}^{+1.12}\times10^{13}$ $\rm 2.34_{-0.79}^{+0.25}$

1153.2719 862.61 unsat

N I
1134.1653 0.00 sat - $24.0\pm2$ > $3.16\times10^{14}$ $\rm 6.80_{-3.05}^{+2.11}$

1134.4149 0.00 sat

1134.9803 0.00 sat

N II
1083.9937 0.00 -^a - $22.0\pm4$ -^a

N II*
1084.5659 48.67 -^a - $22.0\pm4$ -^a

1084.5841 48.67 -^a

N II**
1085.5511 130.80 -^a - $22.0\pm4$ -^a

1085.7096 130.80 -^a

P II
1152.8180 0.00 unsat $\rm -25.37_{-1.25}^{+1.56}$ $1.00_{-0.67}^{+0.65}\times10^{13}$ -^b

P II*
1149.9580 164.90 unsat $\rm -25.37_{-1.25}^{+1.56}$ $1.03_{-0.56}^{+0.74}\times10^{13}$ -^b

P II**
1153.9951 469.12 unsat $\rm -25.37_{-1.25}^{+1.56}$ $1.24_{-0.81}^{+0.70}\times10^{13}$ -^b

Cl I
1097.3691 0.00 unsat $\rm -25.12_{-1.13}^{+1.64}$ $3.12_{-1.53}^{+0.82}\times10^{14}$ -^b

1099.5229 0.00 unsat -^b

**Table 1:** Atomic lines detected in the *FUSE* spectrum of HD 141569A. The velocities are in the pipeline's rest frame (observed spectrum) and are heliocentric. For the saturated lines, we measured the velocity of the centroid; for those lines the error bars on the velocity are symetric (not calculated by a $\chi ^2$ minimization). The radial velocities and line widths have been determined using respectively all the unsaturated and saturated lines of a given ion. "sat'' and "unsat'' are respectively for saturated and unsaturated lines. -^a line not fitted because of the very low S/N ratio of the data; -^b Doppler parameter b not measured because of the unsaturated state of the line.
Element	Wavelength	Energy level	Line	Radial velocity	N	b
	Å	(cm^-1)	State	(km s^-1)	(cm^-2)	(km s^-1)
Ar I	1048.2198	0.00	-^a	- $27.0\pm3$	> $7.30\times10^{14}$	$\rm 5.6_{-0.25}^{+0.42}$
	1066.6599	0.00	sat
FeII	1063.1764	0.00	unsat	$\rm -24.28_{-2.75}^{+1.89}$	$\rm 9.77_{-0.94}^{+4.56}\times10^{15}$	$\rm 2.34_{-0.79}^{+0.25}$
	1096.8770	0.00	sat
	1121.9749	0.00	unsat
	1143.2260	0.00	unsat
	1144.9379	0.00	sat
FeII*	1068.3456	384.79	unsat	$\rm -24.28_{-2.75}^{+1.89}$	$\rm 5.21_{-1.25}^{+3.65}\times10^{13}$	$\rm 2.34_{-0.79}^{+0.25}$
	1096.6073	384.79	unsat
	1147.4092	384.79	unsat
	1148.2773	384.79	unsat
FeII**	1071.5842	667.68	unsat	$\rm -24.28_{-2.75}^{+1.89}$	$4.25_{-2.65}^{+4.36}\times10^{13}$	$\rm 2.34_{-0.79}^{+0.25}$
	1151.1458	667.68	unsat
FeII***	1148.0789	862.61	unsat	-24.28 _-2.75^+1.89	$2.77_{-0.89}^{+1.12}\times10^{13}$	$\rm 2.34_{-0.79}^{+0.25}$
	1153.2719	862.61	unsat
N I	1134.1653	0.00	sat	- $24.0\pm2$	> $3.16\times10^{14}$	$\rm 6.80_{-3.05}^{+2.11}$
	1134.4149	0.00	sat
	1134.9803	0.00	sat
N II	1083.9937	0.00	-^a	- $22.0\pm4$		-^a
N II*	1084.5659	48.67	-^a	- $22.0\pm4$		-^a
	1084.5841	48.67	-^a
N II**	1085.5511	130.80	-^a	- $22.0\pm4$		-^a
	1085.7096	130.80	-^a
P II	1152.8180	0.00	unsat	$\rm -25.37_{-1.25}^{+1.56}$	$1.00_{-0.67}^{+0.65}\times10^{13}$	-^b
P II*	1149.9580	164.90	unsat	$\rm -25.37_{-1.25}^{+1.56}$	$1.03_{-0.56}^{+0.74}\times10^{13}$	-^b
P II**	1153.9951	469.12	unsat	$\rm -25.37_{-1.25}^{+1.56}$	$1.24_{-0.81}^{+0.70}\times10^{13}$	-^b
Cl I	1097.3691	0.00	unsat	$\rm -25.12_{-1.13}^{+1.64}$	$3.12_{-1.53}^{+0.82}\times10^{14}$	-^b
	1099.5229	0.00	unsat			-^b

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observation and data reduction
	3 Results
	4 Discussion
	5 Conclusion
	References