CORDIS Project
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The project develops advanced models to understand dust formation and its impact on stellar winds in aging solar-like stars. It aims to connect the chemistry of gas and dust in the circumstellar environment and explore the potential for planet formation in AGB star disks.
In their twilight years, solar-like stars in the asymptotic giant branch (AGB) phase enrich the interstellar medium (ISM) with fresh material (gas and dust) for new stars and planets. AGB stars lose their outer layers to the ISM through a stellar outflow or wind, forming an extended circumstellar envelope (CSE).
The wind is thought to be dust-driven, with dust grains forming close to the star.
State-of-the-art observations have revealed the composition of the inner CSE, allowing the first identi…
UNIVERSITY OF LEEDS
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