The observations of radial velocities of B8-A0 stars were produced in 1932-1937 with one-prism spectrograph and short camera giving a dispersion of 75{AA}/mm at H{gamma}. When reducing the observations the systematic error as described in our previous paper (I) has been taken into account. From the comparison of the radial velocities of 7 stars in common with two catalogues the systematic correction to our radial velocities was deduced, viz.+0.44+/-1.51km/s in the sense Moore-Simeis. In table XII there are given the final radial velocities for 91 stars with mean value of p.e. equal to +/-3.57km/s. In table XII are given observed velocities for 16 stars with variable radial velocities. Very large velocity of the star HD 161817 leads to the conclusion that this star belongs to the class of high-velocity stars.