A catalogue of 122 wide binaries is presented. The list was compiled by sea
rching for common proper-motion companions to the more than 1200 high-veloc
ity and metal-poor stars of Schuster and collaborators. We study the separa
tions for the wide binaries ((a) > 25 AU), and find that they follow Oepik'
s distribution all the way up to 10 000 AU. A subgroup of them, the ones wi
th the most halo-like orbits, follow Oepik's distribution up to 20 000 AU.
The galactic orbits of all systems are calculated, and galactic orbital par
ameters are used, along with the metallicites, to assign each one to the ol
d thin disk, the thick disk, or the halo population.