  We re-examine the question of condensed neutrino objects (de- generate
neutrino matter) based on new calculations. The potential show-stopper issue of
free-streaming light neutrinos inhibiting galaxy formation is addressed. We
compute the period associated with sim- ple harmonic motion (SHM) of galaxies
embedded within condensed neutrino objects. For observational consequences, we
examine the ro- tational velocities of embedded galaxies using Hickson 88A
(N6978) as the prototype. Finally, we point out that degenerate neutrino
objects repel each other in overlap and we compute directly the repulsive force
between two interesting and relevant configurations. An outstanding issue is
whether the accompanying tidal forces generated by condensed neutrino matter on
embedded galaxies give rise to galactic bulges and halos.
