  We consider the recent results on UHECR (Ultra High Energy Cosmic Ray)
composition and their distribution in the sky from ten EeV energy (the dipole
anisotropy) up to the highest UHECR energies and their clustering maps: UHECR
have been found mostly made by light and lightest nuclei. We summarized the
arguments that favor a few localized nearby extragalactic sources for most
UHECR as CenA, NG 253, M82. We comment also on the possible partial role of a
few remarkable galactic UHECR sources. Finally we revive the eventual role of a
relic neutrino eV mass in dark hot halo (hit by ZeV neutrinos) to explain the
new UHECR clustering events centered around a very far cosmic AGN sources as 3C
454.
