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Table 2

Line fluxes of the molecular hydrogen gas in five regions of the SINFONI field of view.

Line [λrest] RN RS RW RE RC

H 2 1–0 S(3)   [1.95 μm] 20.2 ± 1.29 6.88 ± 1.17 11.4 ± 1.52 14.1 ± 1.62 8.35 ± 3.08
[Si vi]   [1.96 μm] <3.88 <3.52 <4.55 <4.86 <8.88
H 2 1–0 S(2)   [2.03 μm] <5.85 <6.59 <5.51 <7.33 <10.3
H 2 2–1 S(3)   [2.07 μm] <6.41 <3.64 <4.89 <5.90 <8.04
H 2 1–0 S(1)   [2.12 μm] 24.2 ± 0.737 11.6 ± 1.62 19.1 ± 0.659 16.1 ± 0.835 44.6 ± 6.15
Brγ   [2.16 μm] <4.01 <4.01 <4.56 <6.19 <4.55
H 2 1–0 S(0)   [2.22 μm] <6.39 <3.61 <5.63 <7.54 <10.2
H 2 2–1 S(1)   [2.24 μm] <4.73 <6.81 <4.59 <9.09 <10.4

Notes. The fluxes are given in units of × 10-17 erg s-1cm-2. The upper limits indicate the 3σ noise level, measured in the wavelength ranges where we expect to detect the lines. The spectra are extracted in five regions, RN, RS, RW, RE, RC of the field of view shown in Fig. 2. Their sizes correspond to the spatial resolution of the observations (0.52′′).

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