Emission maps from VLT/SINFONI for CO (top), Brγ (middle), and H₂ (bottom), integrated over the peak of each line (Δλ ~ 0.00024 μm). Left panels: the black contour lines represent the continuum emission at 2.08559 μm, the levels are(5, 10, 20, 40, 80, 160) × σ where σ ~ 0.1 erg s⁻¹ cm⁻² μm⁻¹ sr⁻¹. Right panels: represent the continuum-subtracted emission maps, where the continuum subtraction was performed by considering the continuum left (blue-shifted) and right (red-shifted) of each emission line, with the exception of the CO, where only the left (blue-shifted) part was considered. The red circle represents the star in the Gaia DR2 catalogue (Source ID: 5339406246100053888, RA(J2000) = 11h12m18.24s, Dec(J2000) = −58d46m22.5s) used for accurate astrometry of our cubes (the circle around it represents the uncertainty ~ 0.3″). The cyan star represents the suggested position of the star given by Tamura et al. (1997); the circle around it represents the uncertainty ~1.7″. The grey star represents the position of the central source as given by our kinematic study (see Sect. 3.4). In all panels north is up and east is left.