Table 5: Free fitting parameters for the H₉ line. The wavelength difference $\Delta \lambda$ between the narrow component and the broad component is also given. In the first spectrum here are three and in the second spectrum two additional metal lines in the direct vicinity of H₉ that had to be fitted simultaneously to give the correct line profile. Especially for the fitting of many lines, the errors should be treated with caution and should be considered only as formal errors.
sp $A_{\rm n}$ $A_{\rm b}$ ${\rm\sigma_{n}}$ ${\rm\sigma_{b}}$ ${\rm\lambda_{n}}$ ${\rm\lambda_{b}}$ ${\rm\Delta\lambda}$

[electrons] [electrons] [Å] [Å] [Å] [Å] [Å]

1 3316 $\pm$ 84 6489 $\pm$ 127 0.21 $\pm$ 0.01 1.15 3835.37 $\pm$ 0.06 3835.34 $\pm$ 0.09 -0.03 $\pm$ 0.11

2 2520 $\pm$ 66 2846 $\pm$ 83 0.20 $\pm$ 0.01 1.00 3835.38 $\pm$ 0.06 3835.43 $\pm$ 0.11 0.05 $\pm$ 0.13

3 671 $\pm$ 41 486 $\pm$ 48 0.16 $\pm$ 0.01 0.48 $\pm$ 0.05 3835.37 $\pm$ 0.07 3835.49 $\pm$ 0.23 0.12 $\pm$ 0.24

4 124 $\pm$ 19 55 $\pm$ 23 0.14 $\pm$ 0.01 0.40 3835.38 $\pm$ 0.08 3835.45 $\pm$ 0.27 0.07 $\pm$ 0.28

5 101 $\pm$ 13 0.17 $\pm$ 0.02 3835.37 $\pm$ 0.16

6 75 $\pm$ 11 0.14 $\pm$ 0.01 3835.43 $\pm$ 0.13

7 248 $\pm$ 20 0.21 $\pm$ 0.02 3835.40 $\pm$ 0.14

8 458 $\pm$ 32 534 $\pm$ 42 0.19 $\pm$ 0.02 0.81 $\pm$ 0.08 3835.39 $\pm$ 0.09 3835.34 $\pm$ 0.29 -0.05 $\pm$ 0.30

**Table 5:** Free fitting parameters for the H₉ line. The wavelength difference $\Delta \lambda$ between the narrow component and the broad component is also given. In the first spectrum here are three and in the second spectrum two additional metal lines in the direct vicinity of H₉ that had to be fitted simultaneously to give the correct line profile. Especially for the fitting of many lines, the errors should be treated with caution and should be considered only as formal errors.
sp	$A_{\rm n}$	$A_{\rm b}$	${\rm\sigma_{n}}$	${\rm\sigma_{b}}$	${\rm\lambda_{n}}$	${\rm\lambda_{b}}$	${\rm\Delta\lambda}$
	[electrons]	[electrons]	[Å]	[Å]	[Å]	[Å]	[Å]
1	3316 $\pm$ 84	6489 $\pm$ 127	0.21 $\pm$ 0.01	1.15	3835.37 $\pm$ 0.06	3835.34 $\pm$ 0.09	-0.03 $\pm$ 0.11
2	2520 $\pm$ 66	2846 $\pm$ 83	0.20 $\pm$ 0.01	1.00	3835.38 $\pm$ 0.06	3835.43 $\pm$ 0.11	0.05 $\pm$ 0.13
3	671 $\pm$ 41	486 $\pm$ 48	0.16 $\pm$ 0.01	0.48 $\pm$ 0.05	3835.37 $\pm$ 0.07	3835.49 $\pm$ 0.23	0.12 $\pm$ 0.24
4	124 $\pm$ 19	55 $\pm$ 23	0.14 $\pm$ 0.01	0.40	3835.38 $\pm$ 0.08	3835.45 $\pm$ 0.27	0.07 $\pm$ 0.28
5	101 $\pm$ 13		0.17 $\pm$ 0.02		3835.37 $\pm$ 0.16
6	75 $\pm$ 11		0.14 $\pm$ 0.01		3835.43 $\pm$ 0.13
7	248 $\pm$ 20		0.21 $\pm$ 0.02		3835.40 $\pm$ 0.14
8	458 $\pm$ 32	534 $\pm$ 42	0.19 $\pm$ 0.02	0.81 $\pm$ 0.08	3835.39 $\pm$ 0.09	3835.34 $\pm$ 0.29	-0.05 $\pm$ 0.30

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data analysis
	3 Radial and rotational velocity
	4 Line asymmetries on LHS 2034
	5 Chromosphere simulations of LHS 2034
	6 Discussion and conclusions
	References