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From PAHs to Solid Carbon

Published online by Cambridge University Press:  30 March 2011

C. Joblin ,
A.G.G.M. Tielens ,
C. Jäger ,
H. Mutschke ,
T. Henning  and
F. Huisken
C. Jäger
Affiliation:
Max-Planck-Institute for Astronomy, Heidelberg and Institute of Solid State Physics, Friedrich Schiller University, Helmholtzweg 3, 07743 Jena, Germany
H. Mutschke
Affiliation:
Astrophysical Institute and University Observatory, Friedrich Schiller University, Schillergässchen 2-3, 07745 Jena, Germany
T. Henning
Affiliation:
Max-Planck-Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
F. Huisken
Affiliation:
Max-Planck-Institute for Astronomy, Heidelberg and Institute of Solid State Physics, Friedrich Schiller University, Helmholtzweg 3, 07743 Jena, Germany

Abstract

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Carbonaceous grains represent a major component of cosmic dust. The review will summarizenew results in laboratory investigations of carbonaceous dust components. Thenanometer-sized carbon particles are supposed to represent a blend of differentlystructured carbon including graphitic, diamond-like, fullerene-like and chain-likecomponents on a subnanometer or nanometer scale. Recent models used to explain thestructure of gas-phase condensed carbon nano-particles are discussed. Possible formationpathways of carbonaceous grains from molecular components and clusters and the role ofpolycyclic aromatic hydrocarbons (PAHs) and fullerenes are disclosed.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 46: PAHs and the Universe: A Symposium to Celebrate the 25thAnniversary of the PAH Hypothesis , 2011 , pp. 293 - 304
Copyright
© EAS, EDP Sciences 2011

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