Estimating the Turn-Around Radii of Six Isolated Galaxy Groups in the
  Local Universe
  The estimates of the turn-around radii of six isolated galaxy groups in the
nearby universe are presented. From the Tenth Data Release of the Sloan Digital
Sky Survey, we first select those isolated galaxy groups at redshifts $z\le
0.05$ in the mass range of [0.3-1]$\times10^{14}\,h^{-1}M_{\odot}$ whose
nearest neighbor groups are located at distances larger than fiften times their
virial radii. Then, we search for a gravitationally interacting web-like
structure around each isolated group, which appears as an inclined streak
pattern in the anisotropic spatial distribution of the neighbor field galaxies
. Out of 59 isolated groups, only seven are found to possess such web-like
structures in their neighbor zones, but one of them turns out to be NGC 5353/4,
whose turn-around radius was already measured in the previous work and thus
excluded from our analysis. Applying the Turn-around Radius Estimator algorithm
devised by Lee et al. to the identified web-like structures of the remaining
six target groups, we determine their turn-around radii and show that three out
of the six targets have larger turn-around radii than the spherical bound limit
predicted by the Planck cosmology. We discuss possible sources of the apparent
violations of the three groups, including the underestimated spherical
bound-limit due to the approximation of the turn-around mass by the virial
mass.
