The influence of dust properties on the mass loss in pulsating AGB stars

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dc.creatorAndersen, A. C.
dc.creatorHoefner, S.
dc.creatorLoidl, R.
dc.date2001-11-14
dc.date.accessioned2026-07-07T02:01:22Z
dc.date.available2026-07-07T02:01:22Z
dc.descriptionWe are currently studying carbon based dust types of relevance for carbon-rich AGB stars, to obtain a better understanding of the influence of the optical and chemical properties of the grains on the mass loss of the star. An investigation of the complex interplay between hydrodynamics,radiative transfer and chemistry has to be based on a better knowledge of the micro-physics of the relevant dust species.
dc.description4 pages, 2 figures. Proceedings for IAU Colloquium 185 "Radial and Nonradial Pulsations as Probes of Stellar Physics"
dc.identifierhttps://arxiv.org/abs/astro-ph/0111277
dc.identifierhttp://arxiv.org/abs/astro-ph/0111277
dc.identifier2002, ASP Conference Series 259, 542
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3719
dc.subjectAstrophysics
dc.titleThe influence of dust properties on the mass loss in pulsating AGB stars
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