Modelling the spectral energy distribution of galaxies IV. Correcting apparent disk scalelengths and central surface brightnesses for the effect of dust at optical and near-infrared wavelengths

Astronomy and Astrophysics

Volumn 456, Issue 3, 2006, Pages 941-952

  Mollenhoff C ^a   Popescu, C C ^b,c,d   Tuffs, R J ^b,c  

^a UNIVERSITY OF HEIDELBERG   (Germany)

^b MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^c CARNEGIE OBSERVATORIES   (United States)

^d ACADEMY OF ROMANIAN SCIENTISTS   (Romania)

Author keywords

Galaxies: fundamental parameters; Galaxies: photometry; Galaxies: spiral; Galaxies: structure; ISM: dust, extinction; Radiative transfer

Indexed keywords

DUST; GALAXIES; INFRARED RADIATION; RADIATORS; SPECTROPHOTOMETRY; SPECTRUM ANALYSIS; ULTRAVIOLET RADIATION;

GALAXIES: FUNDAMENTAL PARAMETERS; GALAXIES: PHOTOMETRY; GALAXIES: SPIRAL; GALAXIES: STRUCTURE; ISM: DUST; RADIATIVE TRANSFER;

ASTROPHYSICS;

EID: 33748938003     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054727     Document Type: Article

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