Mass Losing Asymptotic Giant Branch Stars And Supergiants
Abstract
This paper presents a summary of four invited and twelve contributed presentations on asymptotic giant branch stars and red supergiants, given over the course of two afternoon splinter sessions at the 19th Cool Stars Workshop. It highlights both recent observations and recent theory, with some emphasis on high spatial resolution, over a wide range of wavelengths. Topics covered include 3D models, convection, binary interactions, mass loss, dust formation and magnetic Velds.
- Publication:
-
19th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (CS19)
- Pub Date:
- September 2016
- DOI:
- 10.5281/zenodo.154075
- arXiv:
- arXiv:1609.07954
- Bibcode:
- 2016csss.confE...5W
- Keywords:
-
- AGB stars;
- Supergiants;
- pulsation;
- models;
- binary stars;
- dust;
- interferometry;
- infrared;
- radio;
- stellar parameters;
- Zenodo community cs19;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- To appear in the proceedings of the 19th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun