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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 10.

Left panel: The color scale shows the peak intensity of the N2H+ components associated with tree G, and the white contour shows the mask (corresponding to T peak > 2.5 K) used to identify the filament studied in Section 3.2. The black contours show the continuum emission at 1.34 mm, at levels [0.5,1.0,1.7,2.5,4.2,5.9] mJy beam−1 (from Sanhueza et al. 2019). The red box indicates the position of the zoomed area shown in the right panel. Right panel: V lsr map of tree G within the white contour of the left panel, with CO emission overlaid in contours (from Li et al. 2020). The contours are computed in the velocity indicated in the bottom-right corner, at levels: for the blue component, [1.08, 1.62, 2.16, 2.7 , 3.78, 4.32, 4.86] Jy beam−1 km s−1; for the red component, [1.33, 1.995, 2.66, 3.99, 5.32, 6.65, 9.31, 10.64, 11.97] Jy beam−1 km s−1. The positions of protostars p2 and p3 are shown with yellow stars in both panels.

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