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Recent Results of Solid-State Spectroscopy

Published online by Cambridge University Press:  21 December 2011

Cornelia Jäger
Affiliation:
Laboratory Astrophysics and Cluster Physics Group, Max Planck Institute for Astronomy and Institute of Solid State Physics, Friedrich-Schiller-Universität Jena, Max-Wien-Platz 1, D-07745 Jena, Germany, Email: [email protected]
Thomas Posch
Affiliation:
Institut für Astronomie, Türkenschanzstraße 17, A-1180 Vienna, Austria
Harald Mutschke
Affiliation:
Astrophysikalisches Institut, Friedrich-Schiller-Universität Jena, Schillergässchen 2-3, D-07745 Jena, Germany
Simon Zeidler
Affiliation:
Astrophysikalisches Institut, Friedrich-Schiller-Universität Jena, Schillergässchen 2-3, D-07745 Jena, Germany
Akemi Tamanai
Affiliation:
Kirchhoff-Institut für Physik, Universität Heidelberg, Im Neuenheimer Feld 227, D-69120 Heidelberg, Germany
Bernard L. de Vries
Affiliation:
Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
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Abstract

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Solid state spectroscopy continues to be an important source of information on the mineralogical composition and physical properties of dust grains both in space and on planetary surfaces. With only a few exceptions, artificially produced or natural terrestrial analog materials, rather than ‘real’ cosmic dust grains, are the subject of solid state astrophysics. The Jena laboratory has provided a large number of data sets characterizing the UV, optical and infrared properties of such cosmic dust analogs. The present paper highlights recent developments and results achieved in this context, focussing on ‘non-standard conditions’ such as very low temperatures, very high temperatures and very long wavelengths.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

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