Fig. 16
Spectra obtained with APEX, and for comparison the SiO(5–4) line extracted from the ALMA data integrated over the source (velocity resolution 2 km s−1). From top to bottom panels: Global ALMA SiO(5–4) line, CS(4–3) emission from the EDE and EVS components, HCN(3–2) emission from the EVS components (and other features possibly related to the HVO component), and HCO+ (3–2) emission from the EVS components.
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