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The distribution of carbonaceous molecules and SiN around the S-type AGB star W Aquilae
Published online by Cambridge University Press: 30 November 2022
Abstract
S-type AGB stars, with C/O ratios close to 1, are expected to have a mixed circumstellar chemistry as they transition from being oxygen-rich stars to carbon-rich stars. Recently, several different carbonaceous molecules, thought to be more characteristic of carbon stars, have been found in the circumstellar envelope of the S-type AGB star W Aql. We have obtained new high spatial resolution ALMA images of some of these molecules, specifically HC3N, SiC2 and SiC, and SiN, which we present here. We report diverse behaviour for these molecules, with SiC2 being seen with a symmetric spatial distribution around the star, SiN and SiC being asymmetrically distributed to the north-east of the star, and HC3N being seen in a broken shell to the south-west. These differing distributions point to complex dynamics in the circumstellar envelope of W Aql.
- Type
- Contributed Paper
- Information
- Proceedings of the International Astronomical Union , Volume 16 , Symposium S366: The Origin of Outflows in Evolved Stars , November 2020 , pp. 178 - 183
- Copyright
- © The Author(s), 2022. Published by Cambridge University Press on behalf of International Astronomical Union
Footnotes
Senior Postdoctoral Fellow of the Fund for Scientific Research (FWO), Flanders, Belgium.