Image Details

Choose export citation format:

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 4.

The green color scale shows the normalized kernel density distribution of σv and N col in AG14, with the contour levels set on [0.1, 0.3, 0.5, 0.7, 0.9]. The same data are shown for AG351 with the dashed contours and for AG354 with solid contours (taken from Redaelli et al. 2021; the N col values have been corrected by a factor ﹩\sqrt{\pi }﹩; see text for details). The horizontal blue solid and red dashed–dotted lines represent the sound speed and the thermal broadening of o‐H2D+, respectively, both at 10 K.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse