Figures and Tables

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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Figure 1 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 1

Model of the molecular outflows in VY CMa, superimposed on the HST infrared image.

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Figure 2

Sample molecular spectra from VY CMa, measured with the Arizona Radio Observatory's Sub-millimeter Telescope (SMT), showing the variation in line profiles.

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Figure 3

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

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Table 1 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Table 1

Molecular abundances in VY Canis Majoris

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