Large Scale Structure in Absorption: Gas within and around Galaxy Voids
  We investigate the properties of the HI Ly-a absorption systems (Ly-a forest)
within and around galaxy voids at z<0.1. We find a significant excess (>99%
c.l.) of Ly-a systems at the edges of galaxy voids with respect to a random
distribution, on ~5 h^{-1} Mpc scales. We find no significant difference in the
number of systems inside voids with respect to the random expectation. We
report differences between both column density (N_{HI}) and Doppler parameter
(b_{HI}) distributions of Ly-a systems found inside and at the edge of galaxy
voids at the >98% and >90% c.l. respectively. Low density environments (voids)
have smaller values for both N_{HI} and b_{HI} than higher density ones (edges
of voids). These trends are theoretically expected and also found in GIMIC, a
state-of-the-art hydrodynamical simulation. Our findings are consistent with a
scenario of at least three types of Ly-alpha: (1) containing embedded galaxies
and so directly correlated with galaxies (referred as `halo-like'), (2)
correlated with galaxies only because they lie in the same over-dense LSS, and
(3) associated with under-dense LSS with a very low auto-correlation amplitude
(~ random) that are not correlated with luminous galaxies. We argue the latter
arise in structures still growing linearly from the primordial density
fluctuations inside galaxy voids that have not formed galaxies because of their
low densities. We estimate that these under-dense LSS absorbers account for
25-30% +- 6% of the current Ly-a population (N_{HI} > 10^{12.5} cm^{-2}) while
the other two types account for the remaining 70-75% +- 12%. Assuming that only
N_{HI} > 10^{14} cm^{-2} systems have embedded galaxies nearby, we have
estimated the contribution of the `halo-like' Ly-a to be ~12-15% +- 4% and
consequently ~55-60% +- 13% of the Ly-a systems to be associated with the
over-dense LSS.
