Dwarf Galaxies in the Halo of NGC 891
  We report the results of a survey of the region within 40 arcmin of NGC 891,
a nearby nearly perfectly edge-on spiral galaxy. Candidate "non-stars" with
diameters greater than 15 arcsec were selected from the GSC 2.3.2 catalog and
cross-comparison of observations in several bands using archived \galex, DSS2,
WISE, and 2MASS images identified contaminating stars, artifacts and background
galaxies, all of which were excluded. The resulting 71 galaxies, many of which
were previously uncataloged, comprise a size limited survey of the region. A
majority of the galaxies are in the background of NGC 891 and are for the most
part members of the Abell 347 cluster at a distance of about 75 \Mpc. The new
finds approximately double the known membership of Abell 347, previously
thought to be relatively sparse. We identify a total of 7 dwarf galaxies, most
of which are new discoveries. The newly discovered dwarf galaxies are dim and
gas-poor and may be associated with the previously observed arcs of RGB halo
stars in the halo and the prominent HI filament and the lopsided features in
the disk of NGC 891. Several of the dwarfs show signs of disruption, consistent
with being remnants of an ancient collision.
