PAH charge state distribution and DIB carriers: Implications from the line of sight toward HD 147889

Astronomy and Astrophysics

Volumn 432, Issue 2, 2005, Pages 515-529

  Ruiterkamp, R ^a   Cox, N L J ^b   Spaans, M ^c   Kaper, L ^b   Foing, B H ^d   Salama, F ^e   Ehrenfreund, P ^b  

^a LEIDEN UNIVERSITY   (Netherlands)

^b Sterrenkundig Institut Anton Pannekoek   (Netherlands)

^c UNIVERSITY OF GRONINGEN   (Netherlands)

^d ESA Research Department   (Netherlands)

^e NASA AMES RESEARCH CENTER   (United States)

Author keywords

ISM: Abundances; ISM: Clouds; ISM: Individual objects: HD 147889; ISM: Molecules

Indexed keywords

ATOMS; CARBON; ELECTRONS; IONIZATION; MOLECULES; SPECTRUM ANALYSIS; STATISTICAL METHODS; ULTRAVIOLET RADIATION;

ABUNDANCES-ISM; CLOUDS-ISM; HD 147889; INDIVIDUAL OBJECTS; ISM;

POLYCYCLIC AROMATIC HYDROCARBONS;

EID: 15244352995     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040331     Document Type: Article

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