Protostellar Outflows at the EarliesT Stages (POETS) VI. Evidence of disk-wind in G11.92-0.61 MM1

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Fig. 1

ALMA 1.3 mm continuum image of MM1a and MM1b. The contour levels are indicated at the bottom of the image with 1σ=~0.1 mJy beam⁻¹ (Table 1). The synthesised beam is indicated as a grey ellipse in the lower-left corner. The blue and red arrows indicate the orientation of the large-scale ¹²CO outflow from Ilee et al. (2016).

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