Sulfur oxides tracing streamers and shocks at low-mass protostellar disk–envelope interfaces

Open Access

Fig. B.2

Upper: Spectrum of SO₂ 16_1,15 – 15_2,14 at position P2 of DK Cha (Fig. 8d), supporting that P1 is a warm (and even hot) spot (Fig. 10). The orange line shows the Gaussian fit. Lower: Same as the upper panel, but for the spectrum smoothed by convolving with a 3-point Flanning window.

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