Resolving the Ultra-Luminous X-ray Sources in the Ly$\alpha$ Emitting
  Galaxy Haro 11
  Lyman continuum and line emission are thought to be important agents in the
reionization of the early universe. Haro 11 is a rare example of a local galaxy
in which Ly$\alpha$ and continuum emission have escaped without being absorbed
or scattered by ambient gas and dust, potentially as a consequence of feedback
from its X-ray sources. We build on our previous Chandra analysis of Haro 11 by
analyzing three new observations. Our subpixel spatial analysis reveals that
the two previously known X-ray sources are each better modelled as ensembles of
at least 2 unresolved point sources. The spatial variability of these
components reveals X1 as a dynamical system where one luminous X-ray source
($L_{\rm X} \sim 10^{41}$ erg s$^{-1}$) fades as a secondary source begins to
flare. These might be intermediate mass black holes or low luminosity active
galactic nuclei near the center of the galaxy in the process of merging.
Optical emission line diagnostics drawn from the literature suggest that while
the galaxy as a whole is consistent with starburst signatures of ionization,
the individual regions wherein the X-ray sources reside are more consistent
with AGN/composite classification. The sources in X2 exhibit some degree of
flux variability. X2a dominates the flux of this region during most
observations ($L_{\rm X} \sim 6\ \times\ 10^{40}$ erg s$^{-1}$), and gives the
only evidence in the galaxy of a soft Ultra-Luminous X-ray source capable of
high energy winds, which we suggest are responsible for allowing the coincident
Ly$\alpha$ emission to escape.
