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Fig. 3
H- and K-band SINFONI spectra of both components of HH 250-IRS. Both sources display a heavily reddened and veiled continuum with emission in the H2 line at 2.122 μm as the only outstanding feature. HH 250-IRS SE, the least reddened of both components, also shows hints of CO absorption starting at 2.293 μm.
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