Hostname: page-component-78c5997874-4rdpn Total loading time: 0 Render date: 2024-11-14T07:26:30.558Z Has data issue: false hasContentIssue false
  • English
  • Français

Amorphous Hydrocarbon Optical Properties

Published online by Cambridge University Press:  05 March 2015

Anthony Jones
Anthony Jones*
Affiliation:
Université Paris Sud & CNRS, Institut d'Astrophysique Spatiale, UMR8617, Orsay, F-91405 email: Anthony.Jones@ias.u-psud.fr
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Hydrogenated amorphous carbon materials, a-C(:H), whose optical properties evolve in response to UV irradiation processing are promising candidate materials for cosmic carbonaceous dust. The optical properties of a:C(:H) particles have been derived as a function of size, band gap and hydrogen content over a wide wavelength range (EUV-cm) and can be used to investigate the size-dependent evolution of a-C(:H) material properties in the ISM.

Keywords

(ISM:) dustextinctionISM: moleculesISM: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 707 - 708
Copyright
Copyright © International Astronomical Union 2015 

References

Bernard-Salas, J., Cami, J., Peeters, E., et al. 2012, ApJ 757, 41CrossRefGoogle Scholar
Jones, A. P. 2009, in Astronomical Society of the Pacific Conference Series, Vol. 414, Cosmic Dust - Near and Far, ed. Henning, T., Grün, E., & Steinacker, J., 473–+Google Scholar
Jones, A. P. 2012a, A&A 542, A98Google Scholar
Jones, A. P. 2012b, A&A 540, A1Google Scholar
Jones, A. P. 2012c, A&A 540, A2Google Scholar
Jones, A. P. & Nuth, J. A. 2011, A&A 530, A44Google Scholar
Micelotta, E. R., Jones, A. P., Cami, J., et al. 2012, ApJ 761, 35CrossRefGoogle Scholar
Serra Díaz-Cano, L. & Jones, A. P. 2008, A&A 492, 127Google Scholar