Morpho-Kinematics of the Circumstellar Environments around Post-AGB Stars
Abstract
We observed two proto-planetary nebulae, HD 56126 representing a source with an elliptical circumstellar shell, and IRAS 16594-4656 representing a source with a bipolar circumstellar shell, with ALMA in the 12CO and 13CO J=3-2 lines and neighboring continuum to see how the morpho-kinematics of CO gas and dust emission properties in their circumstellar environments differ.
- Publication:
-
Why Galaxies Care About AGB Stars: A Continuing Challenge through Cosmic Time
- Pub Date:
- December 2019
- DOI:
- 10.1017/S1743921318006373
- Bibcode:
- 2019IAUS..343..520U
- Keywords:
-
- stars: AGB and post-AGB;
- planetary nebulae: general;
- circumstellar matter;
- stars: mass loss;
- radio lines: stars