The Void Galaxy Survey: Morphology and Star Formation Properties of Void
  Galaxies
  We present the structural and star formation properties of 59 void galaxies
as part of the Void Galaxy Survey (VGS). Our aim is to study in detail the
physical properties of these void galaxies and study the effect of the void
environment on galaxy properties. We use Spitzer 3.6 $\rm{\mu m}$ and B-band
imaging to study the morphology and color of the VGS galaxies. For their star
formation properties, we use Halpha and GALEX near-UV imaging. We compare our
results to a range of galaxies of different morphologies in higher density
environments. We find that the VGS galaxies are in general disk dominated and
star forming galaxies. Their star formation rates are, however, often less than
1 $\rm{M_{\odot}}$ $\rm{yr^{-1}}$. There are two early-type galaxies in our
sample as well. In $\rm{r_{e}}$ versus $\rm{M_{B}}$ parameter space, VGS
galaxies occupy the same space as dwarf irregulars and spirals.
