Carbonaceous dust in interstellar shock waves: Hydrogenated amorphous carbon (a-C:H) vs. graphite

Astronomy and Astrophysics

Volumn 492, Issue 1, 2008, Pages 127-133

  Díaz Cano, L Serra ^a   Jones, A P ^a  

^a CNRS   (France)

Author keywords

ISM: abundances; ISM: dust, extinction; ISM: evolution; ISM: general; Shock waves

Indexed keywords

DUST; EROSION; GAS DYNAMICS; GASES; GRAPHITE; HYDROGENATION; MATERIALS PROPERTIES; SHOCK WAVES; SOIL MECHANICS; WAVES;

CARBON GRAINS; CARBONACEOUS DUSTS; CARBONACEOUS GRAINS; GAS PHASE; GRAIN COLLISIONS; HYDROGENATED AMORPHOUS CARBONS; INTERSTELLAR MEDIUMS; ION IRRADIATIONS; ISM: ABUNDANCES; ISM: DUST, EXTINCTION; ISM: EVOLUTION; ISM: GENERAL; SHOCK MODELS; SPUTTERING EFFECTS; STUDY MATERIALS;

AMORPHOUS CARBON;

EID: 57249115809     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810622     Document Type: Article

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