http://arxiv.org/abs/2204.08944
We have conducted a near-infrared monitoring campaign at the UK InfraRed Telescope (UKIRT), of the Local Group spiral galaxy M33 (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 M33.
A. Javadi and J. Loon
Wed, 20 Apr 22
15/62
Comments: A talk presented at the “IAU symposium 366 : The Origin of Outflows in Evolved Stars”, to be published in the “IAU Proceedings Series”
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