FIGURE 3. Comparison of spectra for the metastable isomers HCN and HNC in VY CMa.

From the following article:

Chemical complexity in the winds of the oxygen-rich supergiant star VY Canis Majoris

L. M. Ziurys, S. N. Milam, A. J. Apponi & N. J. Woolf

Nature 447, 1094-1097(28 June 2007)

doi:10.1038/nature05905

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The J = 3 right arrow 2 rotational transitions of both species are shown in the figure. The HNC spectrum is displayed in red, whereas that for HCN is plotted in black. HNC shows only the red- and blue-shifted flows, whereas HCN has a contribution from the spherical wind as well. The HNC/HCN ratio is roughly 0.001 for the directed flows, indicating high temperature formation26, perhaps due to shocks. The spectra were measured in the 1-mm wavelength band using the SMT. The scale on the left-hand side of the spectra applies to the HCN data, whereas that on the right is for HNC. Spectral resolution for both lines is 1 MHz.

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