  P-Stars are a new class of compact stars made of up and down quarks in
beta-equilibrium with electrons in an Abelian chromomagnetic condensate. We
show that P-Stars are able to account for compact stars with R < 6 Km, as well
as stars with radius comparable with canonical Neutron Stars. We find that
cooling curves of P-Stars compare rather well with observational data. We
suggest that P-Matter produced at the primordial deconfinement transition is a
viable candidate for baryonic Cold Dark Matter. Finally, we show that P-Stars
are able to overcome the gravitational collapse even for mass much greater than
10^6 Solar Mass.
