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High-mass star formation at sub-50 au scales

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Academic year: 2019

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Figure

Fig. 1. Spectra of the four spectral windows extracted toward the main mm continuum peak position mm1
Fig. 2. ALMA 1.3 mm continuum data toward the high-mass star-forming region G351.77-0.54 at an angular resolution of 0bars assuming 1.0of the individual zoom windows
Fig. 3.Color-scaleshowsformm1thefirstmomentmap (intensity-weighted peak velocities) from the line at217.82 GHz
Fig. 4. Channel map of the 217.82 GHz line for mm1. The top-left panel presents the integrated emission between -18 and+14 km s−1
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