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The Core Population and Kinematics of a Massive Clump at Early Stages: An Atacama Large Millimeter/submillimeter Array View

  • Authors: Elena Redaelli, Stefano Bovino, Patricio Sanhueza, Kaho Morii, Giovanni Sabatini, Paola Caselli, Andrea Giannetti, Shanghuo Li

Elena Redaelli et al 2022 The Astrophysical Journal 936 .

  • Provider: AAS Journals

Caption: Figure 5.

In black we show the average o‐H2D+(11,0–11,1) spectra obtained in each core (labeled at the top-right corner of each panel). The red histogram shows the best-fit obtained with MCWEEDS. The corresponding best-fit parameters are recorded in Table 2. Cores that overlap by at least 5% of their extension with another core are marked with a blue asterisk in the top-left corner of the panel.

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