Carbonaceous molecules in the oxygen-rich circumstellar environment of binary post-AGB stars : C60 fullerenes and polycyclic aromatic hydrocarbons

Astronomy and Astrophysics

Volumn 536, Issue , 2011, Pages

  Gielen, C ^a,b   Cami, J ^c,d   Bouwman, J ^b   Peeters, E ^c,d   Min, M ^e  

^a KU LEUVEN   (Belgium)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c UNIVERSITY OF WESTERN ONTARIO   (Canada)

^d SETI INSTITUTE   (United States)

^e UTRECHT UNIVERSITY   (Netherlands)

Author keywords

binaries: general; circumstellar matter; stars: abundances; stars: AGB and post AGB

Indexed keywords

BINARIES: GENERAL; CARBON RICH; CIRCUMSTELLAR; CIRCUMSTELLAR MATTERS; DUST EMISSION; EMISSION FEATURES; EMISSION LINES; EVOLVED STARS; GAS SPECIES; HIGH CRYSTALLINITY; INFRARED BANDS; INFRARED SPECTRUM; MOLECULAR CHEMISTRY; MOLECULAR GAS; POST-AGB; SPITZER; STARS: ABUNDANCES; STARS: AGB AND POST-AGB;

AROMATIC COMPOUNDS; CARBON DIOXIDE; CRYSTALLOGRAPHY; DUST; FULLERENES; HYDROCARBONS; INFRARED SPECTROSCOPY; MINERALOGY; MINERALS; MOLECULES; OXYGEN; POLYCYCLIC AROMATIC HYDROCARBONS; SILICATES;

STARS;

EID: 82955172979     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117961     Document Type: Article

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