Morphological effects on IR band profiles. Experimental spectroscopic analysis with application to observed spectra of oxygen-rich AGB stars
- Autor(en)
- A Tamanai, Harald Mutschke, Thomas Posch
- Abstrakt
Aims. To trace the source of the unique 13, 19.5, and 28 ?m emission features in the spectra of oxygen-rich circumstellar shells around AGB stars, we have compared dust extinction spectra obtained by aerosol measurements. Methods: We have measured the extinction spectra for 19 oxide powder samples of eight different types, such as Ti-compounds (TiO, TiO2, Ti2O3, Ti3O5, Al2TiO5, CaTiO3), ?-, ?-, ?-?-?-Al2O3, and MgAl2O4 in the infrared region (10-50 ?m) paying special attention to the morphological (size, shape, and agglomeration) effects and the differences in crystal structure. Results: Anatase (TiO2) particles with rounded edges are the possible 13, 19.5 and 28 ?m band carriers as the main contributor in the spectra of AGB stars, and spherically shaped nano-sized spinel and Al2TiO5 dust grains are possibly associated with the anatase, enhancing the prominence of the 13 ?m feature and providing additional features at 28 ?m. The extinction data sets obtained by the aerosol and CsI pellet measurements have been made available for public use at elbe.astro.uni-jena.de.
- Organisation(en)
- Institut für Astrophysik
- Externe Organisation(en)
- Friedrich-Schiller-Universität Jena
- Journal
- Astronomy & Astrophysics
- Band
- 501
- Seiten
- 251-267
- Anzahl der Seiten
- 17
- ISSN
- 0004-6361
- Publikationsdatum
- 2009
- Peer-reviewed
- Ja
- ÖFOS 2012
- 1030 Physik, Astronomie, 6031 Philosophie, Ethik
- Link zum Portal
- https://ucrisportal.univie.ac.at/de/publications/2a9c6ff3-fb4b-4b83-9e23-7ba6b2debb03