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Mass–loss rates of cool evolved stars in M 33 galaxy

Published online by Cambridge University Press:  30 November 2022

Atefeh Javadi Open the ORCID record for Atefeh Javadi [Opens in a new window]  and
Jacco Th. van Loon
Atefeh Javadi
Affiliation:
School of Astronomy, Institute for Research in Fundamental Sciences (IPM), P. O. Box 19395-5531, Tehran, Iran email: atefeh@ipm.ir
Jacco Th. van Loon
Affiliation:
Lennard-Jones Laboratories, Keele University, ST5 5BG, UK email: j.t.van.loon@keele.ac.uk
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Abstract

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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.

Keywords

starsevolution–starsmass–loss–galaxiesindividualM 33–galaxiesstar formation
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S366: The Origin of Outflows in Evolved Stars , November 2020 , pp. 210 - 215
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Copyright
© The Author(s), 2022. Published by Cambridge University Press on behalf of International Astronomical Union

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