Simulated infrared emission spectra of highly excited polyatomic molecules: A detailed model of the PAH-UIR hypothesis

Astrophysical Journal

Volumn 493, Issue 2 PART I, 1998, Pages 793-802

  Cook, D J ^a   Saykally, R J ^b  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF PENNSYLVANIA   (United States)

Author keywords

Infrared: ISM: lines and bands; ISM: molecules; Molecular data; Molecular processes; Planetary nebulae: general; Radiation mechanisms: nonthermal

Indexed keywords

CATION; POLYCYCLIC AROMATIC HYDROCARBON;

ARTICLE; ASTRONOMY; CHEMICAL MODEL; INFRARED SPECTROPHOTOMETRY; MATHEMATICS; MICROCLIMATE; NASA DISCIPLINE EXOBIOLOGY; NON-NASA CENTER; PHOTON;

NASA DISCIPLINE EXOBIOLOGY; NON-NASA CENTER;

ASTRONOMY; CATIONS; EXTRATERRESTRIAL ENVIRONMENT; MATHEMATICS; MODELS, CHEMICAL; PHOTONS; POLYCYCLIC HYDROCARBONS, AROMATIC; SPECTROPHOTOMETRY, INFRARED;

EID: 0343096534     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/305156     Document Type: Article

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