Mass-loss rates of cool evolved stars in M 33 galaxy
Abstract
We have conducted a near-infrared monitoring campaign at the UK InfraRed Telescope (UKIRT), of the Local Group spiral galaxy M 33 (Triangulum). In this paper, we present the dust and gas mass-loss rates by the pulsating Asymptotic Giant Branch (AGB) stars and red supergiants (RSGs) across the stellar disc of M 33.
- Publication:
-
The Origin of Outflows in Evolved Stars
- Pub Date:
- 2022
- DOI:
- 10.1017/S1743921322001326
- arXiv:
- arXiv:2204.08944
- Bibcode:
- 2022IAUS..366..210J
- Keywords:
-
- stars;
- evolution-stars;
- mass-loss-galaxies;
- individual;
- M 33-galaxies;
- star formation;
- Astrophysics - Astrophysics of Galaxies;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- A talk presented at the "IAU symposium 366 : The Origin of Outflows in Evolved Stars", to be published in the "IAU Proceedings Series"