CALCULATING SPACE VELOCITIES (U,V,AND W) FOR STARS IN THE HALO OF OUR GALAXY

Space velocities (U,V,and W)for many stars in the halo of our galaxy were calculated by choosing A,G and K spectral type stars at a distance nearly 10 pc. It was found that some of these stars represent a Local Association group (kinematic stream), the stars of this group are sharing in similar 3-D kinematic motion in the galaxy, in the solar neighborhood. The results displayed that these velocities are in a good correlation with each other .