2008MNRAS.386.2290M

Radiative transfer modelling of the Infrared Space Observatory (ISO) spectrum of IRAS22036+5306 has shown that its unusual 11-µm band can be suitably modelled with an alumina-olivine mixture substantially dominated by the former. The results of this work add further credence to recent findings that significant amounts of Al₂O₃ dust grains are present in the dust shells of stars near or beyond the tip of the asymptotic giant branch. Indeed, in the case of IRAS22036+5306, Al₂O₃ dominates the dust composition to the extent that it shifts the 9.8-µm band due to amorphous silicates to 11µm. IRAS22036+5306 may be an unusual case in that the inner dust torus is maintained at a sufficiently high temperature for Al₂O₃ condensation, but not silicate.