Arcsecond resolution images of the chemical structure of the low-mass protostar IRAS 16293-2422 - An overview of a large molecular line survey from the Submillimeter Array

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Fig. 16

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Comparison between ¹³CO 2–1 (upper left), C¹⁸O 2–1 (upper right), H₂CO 3_1,2 − 2_1,1 (lower left) and HCO 3_1,2 − 2_1,1 (lower right). For all species the emission is integrated from 1 to 5 km s^-1. The contours are shown in steps of 9 Jy beam^-1 km s^-1 for the CO isotopologues and 3 Jy beam^-1 km s^-1 for the H₂CO isotopologues.

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