The UK Infrared Telescope M33 monitoring project. VI. Feedback from dusty stellar winds across the galactic disc

arXiv:2607.19989 · astro-ph.GA, astro-ph.SR · Submitted 2026-07-22 · Read on arXiv

Atefeh Javadi, Jacco Th. van Loon, Mina Alizadeh, Seyed Azim Hashemi, Elham Saremi

astro-ph.GA, astro-ph.SR

Submitted: 2026-07-22

Comments: Resubmitted to MNRAS in 2018 after addressing the referee's comments

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Metallicity — 13× in this paper · explained in 3 episodes
• Trace — 5× in this paper · explained in 2 episodes
• Core — 3× in this paper · explained in 2 episodes
• Asymptotic Giant Branch — 2× in this paper
• Consistency — 2× in this paper · explained in 3 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• Large Magellanic Cloud — 1× in this paper
• Luminous Blue Variable — 1× in this paper
• Selection Bias — 1× in this paper · explained in 4 episodes
• Small Magellanic Cloud — 1× in this paper
• Star Formation Rate (SFR) — 1× in this paper · explained in 5 episodes

Sources

• Detection of an OH 1665-MHz Maser in M33
• Millimeter mapping at z~1: dust-obscured bulge building and disk growth
• Spatially resolving the dust properties and submillimetre excess in M 33

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