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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 17.

Left panel: zero moment of the CS map. Dashed contours indicate the −0.03 Jy beam−1 km s−1 level. Right panel: in blue, we show the SEST CS ﹩J=2\to 1﹩ spectrum of IRAS 16562−3959 (Bronfman et al. 1996). The black and green lines show, respectively, the zero-space corrected and uncorrected CS spectra from the ALMA data cubes weighted by the SEST beam. The spectrum in red considers only the positive part of the emission from the ALMA cubes.

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