Fig. 7

Normalized SINFONI H- and K-band spectra of the two brightest stars detected in IRAS 06084-0611. The spectrum of object 1 is characterized by absorption lines of the hydrogen Brackett series. The spectrum of object 2 shows numerous hydrogen lines in emission of which Brγ (2.166 μm) is the most prominent. The spectra of the other objects in the field are shown in Figs. 8 and 9.
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