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 3.

Composite maps obtained showing together the results of MCWEEDS fit on the o‐H2D+ spectra for all the cores. Panel (a): molecular column density, with contours of the 0.8 mm continuum emission overlaid (levels from 2 to 11σ, in steps of 3σ); Panel (b): V lsr map, with the o‐H2D+-identified cores shown in black contours, and numeric labels; Panel (c): velocity dispersion σv map; Panel (d): one-dimensional turbulent Mach number. Note that in case of core overlapping, the maps show the results of only one of them. For the complete sets of maps of each individual core we refer to Appendix. B. The beam size and scale bar are indicated in the bottom left and right corners, respectively, of panel (d).

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse