Image Details

Choose export citation format:

Chemistry of the High-mass Protostellar Molecular Clump IRAS 16562–3959

  • Authors: Andrés E. Guzmán, Viviana V. Guzmán, Guido Garay, Leonardo Bronfman, and Federico Hechenleitner

2018 The Astrophysical Journal Supplement Series 236 45.

  • Provider: AAS Journals

Caption: Figure 12.

Propyne (CH3CCH) physical parameters toward IRAS 16562−3959. The left and right panels show the column density and excitation temperature, respectively. We show in each panel the location of the NW cloud, the N-red cloud, the NEC-wall, the Diffuse Ridge, the position of DR (a), (b), and (c) (black crosses), and continuum sources 8 and 10 (red crosses).

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse