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Fig. 2

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VLT/SINFONI observation of IRAS 06084-0611. Top: Sinfoni 2.16 μm line-map with the object identification numbers sorted by SOFI K-band brightness. The positions of evolutionary class (Lada 1987) 0/I (red asterisks), class II (blue squares) objects and VLA radio detections (green stars, Gómez et al. 2002, see Fig. 1 for all their respective ID numbers) are marked. We do not detect the NIR counterpart of VLA 1 in the SINFONI data. Bottom: three-color image created from the SINFONI line maps with green: H2 (2.12 μm, shocked gas), blue: [Fe ii] (1.644 μm, shocked outflows) and red: Br-γ (2.16 μm, ionized gas). Green H2 and blue [Fe ii] spots are clearly visible, suggesting the presence of outflows and jets, respectively, and thereby tracing active star formation. (Epoch: J2000).

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