Refractive index of hydrocarbon solids

DOI

The properties of hydrogenated amorphous carbon (a-C:H) dust are known to evolve in response to the local conditions. We present an adaptable model for the determination of the optical properties of low-temperature, interstellar a-C:H grains that is based on the fundamental physics of their composition.

Identifier
DOI http://doi.org/10.26093/cds/vizier.35400002
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/540/A2
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/540/A2
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/540/A2
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/540/A2
Provenance
Creator Jones A.
Publisher CDS
Publication Year 2012
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics