The dust effects on galaxy scaling relations
  Accurate galaxy scaling relations are essential for a successful model of
galaxy formation and evolution as they provide direct information about the
physical mechanisms of galaxy assembly over cosmic time. We present here a
detailed analysis of a sample of nearby spiral galaxies taken from the KINGFISH
survey. The photometric parameters of the morphological components are obtained
from bulge-disk decompositions using GALFIT data analysis algorithm, with
surface photometry of the sample done beforehand. Dust opacities are determined
using a previously discovered correlation between the central face-on dust
opacity of the disk and the stellar mass surface density. The method and the
library of numerical results previously obtained are used to correct the
measured photometric and structural parameteres for projection (inclination),
dust and decomposition effects in order to derive their intrinsic values.
Galaxy disk scaling relations are then presented, both the measured (observed)
and the intrinsic (corrected) ones, in the optical regime, to show the scale of
the biases introduced by the aforementioned effects. The slopes of the
size-luminosity relations and the dust vs stellar mass are in agreement with
values found in other works. We derive mean dust optical depth and dust/stellar
mass ratios of the sample, which we find to be consistent with previous studies
of nearby spiral galaxies. While our sample is rather small, it is sufficient
to quantify the influence of galaxy environment (dust, in this case) when
deriving scaling relations.
