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Volumn 484, Issue 3, 2008, Pages 631-653

Modelling the spectral energy distribution of ULIRGs. II. the energetic environment and the dense interstellar medium

Author keywords

Galaxies: active; Infrared: galaxies; ISM: dust, extinction; Radio continuum: galaxies

Indexed keywords

CHEMICAL MODIFICATION; CURVE FITTING; ELECTRIC POWER DISTRIBUTION; ENERGY EFFICIENCY; FORMING; GALAXIES; GASES; INFRARED DEVICES; ION BEAMS; LUMINANCE; MATHEMATICAL MODELS; MOLECULAR INTERACTIONS; MOLECULAR STRUCTURE; NEON; OPTICAL PROPERTIES; POLYCYCLIC AROMATIC HYDROCARBONS; POPULATION STATISTICS; RADIATION; SPECTRUM ANALYSIS;

EID: 44849091191     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078883     Document Type: Article
Times cited : (118)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.