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20042008
most citedTracing the development of dust around evolved stars: The case of 47 Tuc

68 citations · 120 across the 3 of their papers we have counts for

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astro-ph200819 cited

Far-infrared spectra of hydrous silicates at low temperatures - Providing laboratory data for Herschel and ALMA

H. Mutschke, S. Zeidler, Th. Posch +3

Hydrous silicates occur in various cosmic environments, and are among the minerals with the most pronounced bands in the far infrared (FIR) spectral region. Given that Herschel and…

astro-ph200733 cited

Carbonates in space - The challenge of low temperature data

Th. Posch, A. Baier, H. Mutschke +1

Carbonates have repeatedly been discussed as possible carriers of stardust emission bands. However, the band assignments proposed so far were mainly based on room temperature powde…

astro-ph200668 cited

Tracing the development of dust around evolved stars: The case of 47 Tuc

T. Lebzelter, T. Posch, K. Hinkle +2

We observed mid-infrared (7.5-22 mum) spectra of AGB stars in the globular cluster 47 Tuc with the Spitzer telescope and find significant dust features of various types. Comparison…

astro-ph2005

Infrared extinction by homogeneous particle aggregates of SiC, FeO and SiO2: comparison of different theoretical approaches

Anja C. Andersen, Harald Mutschke, Thomas Posch +2

Particle shape and aggregation have a strong influence on the spectral profiles of infrared phonon bands of solid dust grains. Calculating these effects is difficult due to the oft…

astro-ph2005

Infrared Extinction by Aggregates of SiC Particles

Anja C. Andersen, Harald Mutschke, Thomas Posch

Particle shape and aggregation have a strong influence on the spectral profiles of infrared phonon bands of solid dust grains. In this paper, we use a discrete dipole approximation…

astro-ph2004

Reconsidering the origin of the 21 micron feature: Oxides in carbon-rich PPNe?

Thomas Posch, Harald Mutschke, Anja C. Andersen

The origin of the so-called "21 micron" feature which is especially prominent in the spectra of some carbon-rich protoplanetary nebulae (PPNe}) is the matter of a lively debate. A…