Fig. C.1
Mass density map obtained using the temperature and continuum maps in Eq. (2). The solid contours correspond to our continuum observations in the AB configuration, starting at 6σ and increasing in steps of 3σ (1σ = 2.5 mJy beam−1). Each of the peak continuum positions, as depicted by stars, is expected to host at least one 10 M⊙ (proto)star or more lower mass sources.
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