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Predictions of variable mass loss for Luminous Blue Variables
Jorick S. Vink, Alex de Koter
We present radiation-driven wind models for Luminous Blue Variables (LBVs) and predict their mass-loss rates. We study the effects of lower masses and modified abundances in compar…
The absence of the 10 um silicate feature in the isolated Herbig Ae star HD 100453
G. Meeus, J. Bouwman, C. Dominik +2
We analyse the optical and IR spectra, as well as the spectral energy distribution (UV to mm) of the candidate Herbig Ae star HD100453. This star is particular, as it shows an ener…
An atlas of 2.4 to 4.1 microns ISO/SWS spectra of early-type stars
A. Lenorzer, B. Vandenbussche, P. Morris +5
We present an atlas of spectra of O- and B-type stars, obtained with the Short Wavelength Spectrometer (SWS) during the Post-Helium program of the Infrared Space Observatory (ISO).…
Dust and the spectral energy distribution of the OH/IR star OH 127.8+0.0: Evidence for circumstellar metallic iron
F. Kemper, A. de Koter, L. B. F. M. Waters +2
We present a fit to the spectral energy distribution of OH 127.8+0.0, a typical asymptotic giant branch star with an optically thick circumstellar dust shell. The fit to the dust s…