  It is shown that a small contamination of a relativistically hot electron
component can induce a new scale (for structure formation) to a system
consisting of an ion-degenerate electron plasma. Mathematically expression of
this additional scale length is the increase in the index of quasi-equilibrium
Beltrami-Bernoulli states that have been invoked to model several astrophysical
systems of interest. The two species of electrons, due to different origin of
their relativistic effective masses, behave as two distinct components (each
with its own conserved helicity) and add to the richness of the accessible
quasi equilibrium states. Determined by the concrete parameters of the system,
the new macro-scale lengths (much larger than the short intrinsic scale lengths
(skin depths) and generally much shorter than the system size) open new
pathways for energy transformations.
