Is the Galactic submillimeter dust emissivity underestimated?

Astronomy and Astrophysics

Volumn 437, Issue 2, 2005, Pages 447-456

  Dasyra, K M ^a,b   Xilouris, E M ^c   Misiriotis, A ^b   Kylafis, N D ^b,d  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b UNIVERSITY OF CRETE   (Greece)

^c NATIONAL OBSERVATORY OF ATHENS   (Greece)

^d INSTITUTE OF COMPUTER SCIENCE   (Greece)

Author keywords

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

Indexed keywords

COMPUTER SIMULATION; GALAXIES; MATHEMATICAL MODELS; PARAMETER ESTIMATION; SUBMILLIMETER WAVES; THICKNESS MEASUREMENT;

EXTINCTION-GALAXIES; GALAXIES-SUBMILLIMETER; ISM; ISM-GALAXIES; SPIRAL-INFRARED;

DUST;

EID: 21644458578     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20042442     Document Type: Article

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