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Fig. 3

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Spectral line fits for H2, HD, and the [S I], [Fe I], and [Fe II] atomic lines for HH 211 aperture 8. The line flux (shaded blue region) is determined by the simultaneous fit of a Gaussian profile and a first order polynomial to represent the continuum. the rest-frame wavelength of each spectral line is shown by a dashed gray line, and non-detections are shown without a shaded region for the fit. Nearby molecular lines of are labeled.

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