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The Mineralogy of Interstellar and Circumstellar Dust in Galaxies

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Astromineralogy

Part of the book series: Lecture Notes in Physics ((LNP,volume 815))

Abstract

Dust in space is ubiquitous and is part of the cycle of matter in galaxies. The observed properties of dust change as a function of the astrophysical environment in which it is found. Dust can therefore be used as a tracer and probe of the physical and chemical conditions where it is detected. We present an observational overview of interstellar and circumstellar dust using spectroscopy at infrared wavelengths. Thanks to the contributions made by space-based infrared spectrographs, a large observational database of dust in space is now available. In this review, we focus on the identification of solid state resonances at these wavelengths, and present an inventory of dust species in different astrophysical environments. The picture that emerges is that of a very rich circumstellar dust mineralogy, while the interstellar medium shows only a limited amount of species. The implications for our understanding of dust processing in different astrophysical environments are also discussed.

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Acknowledgement

We would like to thank Sacha Hony, Jan Cami, Jeroen Bouwman, Jolanda van Breemen, Clio Gielen, Henrik Spoon and Frans Rietmeijer for the supply of several figures and Sacha Hony also for the careful reading of the manuscript. We thank Chiyoe Koike, John Bradley, and our colleagues in Amsterdam, Groningen, Leuven and Jena for the numerous discussions about dust in space and in the laboratory. This overview would not have been possible without the help of ADS and Simbad.

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  1. Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Anna van Saksenlaan 51, 2593 HW, Den Haag, The Netherlands

    F.J. Molster

  2. Nederlandse Onderzoekschool Voor Astronomie (NOVA), Leiden Observatory, Niels Bohrweg 2, 2333, CA, Leiden, The Netherlands

    F.J. Molster

  3. Astronomical Institute “Anton Pannekoek”, University of Amsterdam, Kruislaan 403, 1098 SJ, Amsterdam, The Netherlands

    L.B.F.M. Waters

  4. Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200D, B-3001, Heverlee, Belgium

    L.B.F.M. Waters

  5. Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, The Alan Turing Building, Manchester, M13 9PL, UK

    F. Kemper

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  1. MPI für Astronomie, Königstuhl 17, Heidelberg, 69117, Germany

    Thomas Henning

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Molster, F., Waters, L., Kemper, F. (2010). The Mineralogy of Interstellar and Circumstellar Dust in Galaxies. In: Henning, T. (eds) Astromineralogy. Lecture Notes in Physics, vol 815. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-13259-9_3

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