Arcsecond resolution mapping of sulfur dioxide emission in the circumstellar envelope of VY Canis Majoris

We report Submillimeter Array observations of SO2 emission in the circumstellar envelope (CSE) of the red supergiant VY Canis Majoris, with an angular resolution of 1″. SO2 emission appears in three distinct outflow regions surrounding the central continuum peak emission that is spatially unresolved. No bipolar structure is noted in the sources. A fourth source of SO2 is identified as a spherical wind centered at the systemic velocity. We estimate the SO2 column density and rotational temperature assuming local thermal equilibrium (LTE) as well as perform non-LTE radiative transfer analysis using RADEX. Column densities of SO2 are found to be 10¹⁶cm^-2 in the outflows and in the spherical wind. Comparison with existing maps of the two parent species OH and SO shows the SO2 distribution to be consistent with that of OH. The abundance ratio is greater than unity for all radii larger than 3 × 10 ¹⁶cm. SO2 is distributed in fragmented clumps compared to SO, PN, and SiS molecules. These observations lend support to specific models of circumstellar chemistry that predict and may suggest the role of localized effects such as shocks in the production of SO2 in the CSE. © 2012. The American Astronomical Society. All rights reserved.

Duke Scholars

Author Ken H Young Pathology