Fig. 1
Integrated hyperfine intensity anomalies of the inner satellite lines (left panel) and the outer satellite lines (right panel) derived from 1383 spectra with an S/N larger than 15 in the Integral-Shaped Filament (ISF) of the Orion A molecular cloud. The blue cross in each panel illustrates the location of the Orion Kleinmann-Low Nebula (RA 05:35:14.16 Dec -05:22:21.5 J2000).
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