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Table 2

Emission lines.

Center sp(A) sp(B)

Line Flux FWHM Flux FWHM Flux FWHM
λ [μm] [10-18 W m-2] [km s-1] [10-18 W m-2] [km s-1] [10-18 W m-2] [km s-1]

[Fe ii] 1.94 ± 0.47 190 ± 50 ... ... ... ...
1.644
H2(10)S(3) 1.33 ± 0.13 210 ± 20 0.33 ± 0.02 180 ± 15 0.29 ± 0.02 230 ± 15
1.957
H2(10)S(1) 0.86 ± 0.11 180 ± 25 0.28 ± 0.02 125 ± 10 0.28 ± 0.03 255 ± 25
2.122
Brγ 0.295 ± 0.095 185 ± 70 ... ... ... ...
2.166
H2(10)S(0) 0.36 ± 0.09 230 ± 75 0.065 ± 0.02 190 ± 70 0.05 ± 0.02 195 ± 115
2.223
H2(21)S(1) 0.13 ± 0.06 110 ± 55 0.04 ± 0.015 140 ± 60 0.04 ± 0.02 235 ± 50
2.247
H2(10)Q(1) 1.08 ± 0.20 185 ± 30 0.28 ± 0.03 155 ± 15 0.21 ± 0.04 250 ± 40
2.408
H2(10)Q(2) 0.79 ± 0.265 290 ± 75 ... ... 0.06 ± 0.02 115 ± 35
2.414
H2(10)Q(3) 1.02 ± 0.20 205 ± 30 0.23 ± 0.015 135 ± 15 0.18 ± 0.02 235 ± 35
2.422

Notes. For center: the lines were measured in a 1″ radius aperture centered on the adopted galactic center and nuclear position. For sp(A) and sp(B): the lines were measured in a radius aperture centered on the emission region. See also Fig. 3g. The FWHM is not corrected for instrumental broadening, which is ~100 km s-1 in H-band and ~75 km s-1 in K-band.

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