Modelling the spectral energy distribution of galaxies: V. the dust and PAH emission SEDs of disk galaxies

Astronomy and Astrophysics

Volumn 527, Issue 14, 2011, Pages

  Popescu, C C ^a   Tuffs, R J ^b   Dopita, M A ^c   Fischera, J ^c   Kylafis, N D ^d,e   Madore, B F ^f  

^a UNIVERSITY OF CENTRAL LANCASHIRE   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^c AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^d UNIVERSITY OF CRETE   (Greece)

^e INSTITUTE OF COMPUTER SCIENCE   (Greece)

^f CARNEGIE OBSERVATORIES   (United States)

Author keywords

dust extinction; galaxies: individual: NGC 891; galaxies: spiral; infrared: galaxies; radiative transfer; ultraviolet: galaxies

Indexed keywords

ANGULAR SIZES; DIFFERENT GEOMETRY; DISK GALAXIES; DUST EMISSION; DUST GRAINS; DUST OPACITY; FAR-INFRARED; FORMATION RATES; FREE PARAMETERS; GALAXIES: INDIVIDUALS; GALAXIES: SPIRAL; GEOMETRICAL CONSTRAINTS; HIGHER RESOLUTION; INFRARED: GALAXIES; MASSIVE STARS; MATHEMATICAL FORMS; MIDINFRARED; MODEL PREDICTION; MOLECULAR CLOUDS; MOLECULAR GAS; NON-PARAMETRIC TEST; OBSERVATIONAL DATA; OBSERVED QUANTITY; OPTICAL IMAGE; PAH EMISSIONS; PARAMETER SPACES; PHOTON FIELDS; PHYSICAL PARAMETERS; POPULATION SYNTHESIS; POSTERIORI; PREDICTIVE POWER; RADIATION FIELD; RADIATION TRANSFER; RADIATIVE TRANSFER CALCULATIONS; SELF-CONSISTENT MODEL; SIMULATED DUST; SPECTRAL ENERGY DISTRIBUTION; SPIRAL GALAXIES; STAR FORMING GALAXY; STAR-FORMING REGION; STATISTICAL SURVEY; STELLAR POPULATIONS; STOCHASTIC HEATING; SUBMILLIMETERS; SURFACE BRIGHTNESS; ULTRA-VIOLET; ULTRAVIOLET: GALAXIES; UV LIGHT;

CLOUDS; COLOR; COMPUTER SIMULATION; DUST; ELECTRIC POWER DISTRIBUTION; FORECASTING; GEOMETRICAL OPTICS; GEOMETRY; HEATING; LUMINANCE; POPULATION DISTRIBUTION; POPULATION STATISTICS; RADIATIVE TRANSFER; SPECTROSCOPY; STARS; STOCHASTIC MODELS;

GALAXIES;

EID: 79551698816     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015217     Document Type: Article

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