FAUST - XV. A disc wind mapped by CH3OH and SiO in the inner 300 au of the NGC 1333 IRAS 4A2 protostar

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Fig. D.3.

SiO PV diagrams extracted at the region shown in Figure D.1 and labelled at the top of each plot. The contours are at (3,5,10, 20) σ_s with σ_s∼1.5 mJy beam⁻¹. The vertical and horizontal dashed lines represent the v_sys (∼6.8 km s⁻¹; Choi 2001), and the 0″ offset (on the 4A2 protostar), respectively.

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