The complexity of Orion: an ALMA view - I. Data and first results

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Fig. 7

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CR/MF1 display of expected n-C₃H₇CN components. Despite the coincidental emission peak towards CR/MF1 in Fig. 6 that is visible in the 236.99 GHz window, n-C₃H₇CN is not detected in this source at a similar level to that seen in IRc21 (Fig. 4). Color-coding and T_MB scale as in Fig. 4.

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