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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 2.

Zero-moment maps of the emission from representative transitions from the central 23″ × 23″ region of IRAS 16562−3959. All of these transitions show a strong, dominating source consistent with the position of G345.49+1.47 (Source 10). The upper-left panel shows the continuum measured at 3 mm in a different color scale, together with the sources identified in Paper I. The name of several continuum sources are indicated in the first panel, and their positions are marked in the rest. The dashed contour level in the panels is −0.03 Jy beam−1 km s−1, corresponding to approximately −5σ. The dashed contours in the upper-left panel correspond to those presented in Paper I.

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