Testing the "strong" PAHs hypothesis II. A quantitative link between DIBs and far-IR emission features

Astronomy and Astrophysics

Volumn 410, Issue 2, 2003, Pages 639-648

  Mulas, G ^a   Malloci, G ^a,b   Benvenuti, P ^b,c  

^a INAF OSSERVATORIO ASTRONOMICO DI CAGLIARI   (Italy)

^b UNIVERSITY OF CAGLIARI   (Italy)

^c STECF   (Germany)

Author keywords

Astrochemistry; Infrared: ISM; ISM: lines and bands; ISM: molecules; Line: identification; Molecular processes

Indexed keywords

BAND STRUCTURE; ELECTRONIC STRUCTURE; GALAXIES; MATHEMATICAL MODELS; POLYCYCLIC AROMATIC HYDROCARBONS; SUBSTITUTION REACTIONS;

ELECTRONIC TRANSITION; INFRARED EMISSION BANDS; INTERSTELLAR MEDIUM; ISOTOPIC SUBSTITUTIONS; SKELETAL BANDS; UNIDENTIFIED INFRARED BANDS;

ASTROPHYSICS;

EID: 0242323589     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031212     Document Type: Article

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