UV irradiated hydrogenated amorphous carbon (HAC) materials as a carrier candidate of the interstellar UV bump at 217.5 nm

Astronomy and Astrophysics

Volumn 528, Issue , 2011, Pages

  Gadallah, K A K ^a,b   Mutschke, H ^a   Jager C ^a  

^a FRIEDRICH SCHILLER UNIVERSITY JENA   (Germany)

^b Assiut Branch   (Egypt)

Author keywords

dust, extinction; ISM: lines and bands; methods: laboratory; ultraviolet: ISM

Indexed keywords

ATOMIC STRUCTURE; CARBONACEOUS DUST; CARBONACEOUS NANOPARTICLES; DUST , EXTINCTION; GRAPHENE LAYERS; HIGH VACUUM; HYBRIDIZATION RATIO; HYDROGEN CONTENTS; HYDROGENATED AMORPHOUS CARBON; INTERNAL STRUCTURE; INTERSTELLAR CARBON; INTERSTELLAR DUST; INTERSTELLAR MEDIUMS; ISM: LINES AND BANDS; METHODS: LABORATORY; NANO-SIZED; SPECTRAL FEATURE; SPECTRAL PROPERTIES; STRUCTURAL AND OPTICAL PROPERTIES; TRANSMISSION ELECTRON MICROSCOPE; ULTRAVIOLET: ISM; UV DOSE; UV IRRADIATION; UV RADIATION;

ABLATION; AMORPHOUS CARBON; AMORPHOUS FILMS; DUST; GRAPHENE; HYDROGENATION; IRRADIATION; OPTICAL CORRELATION; OPTICAL PROPERTIES; RADIATION; SPECTROSCOPIC ANALYSIS; TRANSMISSION ELECTRON MICROSCOPY; ULTRAVIOLET RADIATION; VACUUM APPLICATIONS;

MATERIALS PROPERTIES;

EID: 79952163592     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015542     Document Type: Article

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