Tol 2240–384 – a new low-metallicity AGN candidate

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Table 6:

Broad components of strong emission lines.
	UVES		FORS (medium)
Line	Flux^a	FWHM^b	Flux^a	FWHM^b
4340 H $\gamma$	...	...	1.2 $\pm$ 0.1	2500 $\pm$ 200
4861 H $\beta$	13.3 $\pm$ 3.0	380 $\pm$ 100	5.0 $\pm$ 0.1	864 $\pm$ 19
	17.2 $\pm$ 3.0	1050 $\pm$ 300	8.0 $\pm$ 0.1	3993 $\pm$ 93
6563 H $\alpha$	94.7 $\pm$ 0.4	709 $\pm$ 5	47.3 $\pm$ 0.2	590 $\pm$ 5
	169.1 $\pm$ 0.4	2320 $\pm$ 23	87.2 $\pm$ 0.3	2619 $\pm$ 37

Notes. ^(a) Observed flux in units 10^-16 erg s^-1 cm^-2; ^(b) in km s^-1.

Source LaTeX | All tables | In the text

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