Fig. 6
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Correlations between the extinction corrected flux of the HD R(6) line measured in all apertures for our sample with the extinction corrected flux of various atomic and H2 lines. The line flux is related to the line intensity by a constant factor of the aperture solid angle (see text). Top row: correlation with the [S I], [Fe I], and [Fe II] line flux. Bottom row: correlation with the H2 S(1), S(4), and S(7) line flux.
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