Radiative transfer modelling of the Infrared Space Observatory (ISO) spectrum of IRAS 22036+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 wo
In this paper we have investigated the spectrophotometric properties of the Asymptotic Giant Branch ...
Analysis of the low resolution UV(IUE) spectra (1150 to 3200 Å) of 15 hot post-AGB candidates is pr...
In this article we report further investigations of the IRAS selected sample of Planetary Nebula (PN...
This work reports high-resolution spectroscopic stellar parameters and abundance analysis of the pos...
We present a detailed chemical analysis on the basis of high-resolution, high signal-to-noise optica...
We present a revised model for the infrared emission of the hyperluminous infrared galaxy IRAS F1021...
Aims. We focus here on one particular and poorly studied object, IRAS 11472–0800. It is a highly evo...
We present an analysis of our extensive data-set on IRAS 08544–4431. It is the first object we disc...
We present the $\rm{2{-}200{\ }\mu}$m Infrared Space Observatory (ISO) spectrum and $\rm{3.8{-}20{...
We present a new model for the infrared emission of the high redshift hyperluminous infrared galaxy ...
We present an investigation of the dust formation process in the atmospheres of the oxygen-rich AGB ...
The presence of amorphous Al2O3 in the shells of five OH/IR stars has been investigated via radiativ...
We have obtained Johnson U, B, V and Cousins R, I photometry and low resolution spectra of a small ...
Context. The Class 0 protostellar binary IRAS 16293–2422 is an interesting target for (sub)millimete...
We investigate models for the IRAS LRS)Low Resolution Spectra) of OH/IR stars. OH/IR stars often sho...
In this paper we have investigated the spectrophotometric properties of the Asymptotic Giant Branch ...
Analysis of the low resolution UV(IUE) spectra (1150 to 3200 Å) of 15 hot post-AGB candidates is pr...
In this article we report further investigations of the IRAS selected sample of Planetary Nebula (PN...
This work reports high-resolution spectroscopic stellar parameters and abundance analysis of the pos...
We present a detailed chemical analysis on the basis of high-resolution, high signal-to-noise optica...
We present a revised model for the infrared emission of the hyperluminous infrared galaxy IRAS F1021...
Aims. We focus here on one particular and poorly studied object, IRAS 11472–0800. It is a highly evo...
We present an analysis of our extensive data-set on IRAS 08544–4431. It is the first object we disc...
We present the $\rm{2{-}200{\ }\mu}$m Infrared Space Observatory (ISO) spectrum and $\rm{3.8{-}20{...
We present a new model for the infrared emission of the high redshift hyperluminous infrared galaxy ...
We present an investigation of the dust formation process in the atmospheres of the oxygen-rich AGB ...
The presence of amorphous Al2O3 in the shells of five OH/IR stars has been investigated via radiativ...
We have obtained Johnson U, B, V and Cousins R, I photometry and low resolution spectra of a small ...
Context. The Class 0 protostellar binary IRAS 16293–2422 is an interesting target for (sub)millimete...
We investigate models for the IRAS LRS)Low Resolution Spectra) of OH/IR stars. OH/IR stars often sho...
In this paper we have investigated the spectrophotometric properties of the Asymptotic Giant Branch ...
Analysis of the low resolution UV(IUE) spectra (1150 to 3200 Å) of 15 hot post-AGB candidates is pr...
In this article we report further investigations of the IRAS selected sample of Planetary Nebula (PN...
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