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Fig. 4

image

Lines of vinyl acetate, CH3COOCHCH2, towards the compact ridge of Orion KL. The black histogram is the averaged spectrum over 5 × 5 pixels around the methyl acetate peak (see text) of the ALMA SV data (see text for references); these data have a 0.5 MHz of spectral resolution. The thin red line is the synthetic spectrum assuming a column density of 2 × 1015 cm-2 for vinyl acetate (A+E species). The thin blue line is the model for vinyl acetate with a column density of 1 × 1015 cm-2 (A+E species); this model corresponds to the given column density for the tentative detection of vinyl acetate (see text). A vLSR of 7 km s-1 is assumed.

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