{ "id": "1003.3100", "version": "v1", "published": "2010-03-16T08:13:04.000Z", "updated": "2010-03-16T08:13:04.000Z", "title": "Determining the forsterite abundance of the dust around Asymptotic Giant Branch stars", "authors": [ "B. L. de Vries", "M. Min", "L. B. F. M. Waters", "J. A. D. L. Blommaert", "F. Kemper" ], "comment": "Accepted for publication in A&A", "categories": [ "astro-ph.SR" ], "abstract": "Aims. We present a diagnostic tool to determine the abundance of the crystalline silicate forsterite in AGB stars surrounded by a thick shell of silicate dust. Using six infrared spectra of high mass-loss oxygen rich AGB stars we obtain the forsterite abundance of their dust shells. Methods. We use a monte carlo radiative transfer code to calculate infrared spectra of dust enshrouded AGB stars. We vary the dust composition, mass-loss rate and outer radius. We focus on the strength of the 11.3 and the 33.6 \\mu m forsterite bands, that probe the most recent (11.3 \\mu m) and older (33.6 \\mu m) mass-loss history of the star. Simple diagnostic diagrams are derived, allowing direct comparison to observed band strengths. Results. Our analysis shows that the 11.3 \\mu m forsterite band is a robust indicator for the forsterite abundance of the current mass-loss period for AGB stars with an optically thick dust shell. The 33.6 \\mu m band of forsterite is sensitive to changes in the density and the geometry of the emitting dust shell, and so a less robust indicator. Applying our method to six high mass-loss rate AGB stars shows that AGB stars can have forsterite abundances of 12% by mass and higher, which is more than the previously found maximum abundance of 5%.", "revisions": [ { "version": "v1", "updated": "2010-03-16T08:13:04.000Z" } ], "analyses": { "keywords": [ "asymptotic giant branch stars", "forsterite abundance", "mass-loss oxygen rich agb", "mass-loss rate agb stars", "oxygen rich agb stars" ], "tags": [ "journal article" ], "publication": { "doi": "10.1051/0004-6361/200913588", "journal": "Astronomy and Astrophysics", "year": 2010, "month": "Jun", "volume": 516 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 849063, "adsabs": "2010A&A...516A..86D" } } }