Discovery of an old photoevaporating disk in σ Orionis | A&A

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Table 1:

Characteristics of the emission lines.
Line	$\lambda$	pEW	FWHM	Luminosity
	(Å)	(Å)	( $\rm {km ~~ s^{-1}}$ )	10^-5 $L_\odot$
H $\alpha$	6562.71	-15.2 $\pm$ 0.1	69.9 $\pm$ 2	12.0 $\pm$ 0.1
$[\rm {NII}]$	6548.05	-0.82 $\pm$ 0.2	42.6 $\pm$ 1	0.6 $\pm$ 0.15
$[\rm {NII}]$	6583.45	-2.46 $\pm$ 0.1	39.6 $\pm$ 0.5	1.9 $\pm$ 0.1
$[\rm {SII}]$	6716.44	-1.22 $\pm$ 0.03	48.7 $\pm$ 0.4	0.6 $\pm$ 0.02
$[\rm {SII}]$	6730.82	-1.60 $\pm$ 0.08	43.2 $\pm$ 0.4	0.8 $\pm$ 0.04

Source LaTeX | All tables | In the text