The emissivity of dust grains in spiral galaxies

Astronomy and Astrophysics

Volumn 425, Issue 1, 2004, Pages 109-120

  Alton, P B ^a   Xilouris, E M ^b   Misiriotis, A ^c   Dasyra, K M ^d   Dumke, M ^e  

^a Le Mas Fleuri ^*  (France)

^b NATIONAL OBSERVATORY OF ATHENS   (Greece)

^c UNIVERSITY OF CRETE   (Greece)

^d MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^e MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

Author keywords

Galaxies: ISM; Galaxies: spiral; Infrared: galaxies; ISM: dust, extinction; Submillimeter

Indexed keywords

APPROXIMATION THEORY; BOLOMETERS; COMPUTER SIMULATION; COMPUTER SOFTWARE; CORRELATION METHODS; DUST; EXTRAPOLATION; HEAT RADIATION; IMAGE PROCESSING; INFRARED RADIATION; MATHEMATICAL MODELS; SILICATES;

GALAXIES:ISM; INFRARED:GALAXIES; ISM:DUST, EXTINCTION; RADIATION TRANSFER; SUBMILLIMETER;

GALAXIES;

EID: 4744348285     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040438     Document Type: Article

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