)  ![[*Panels a, b, c:*]{} The H[$\alpha$]{} region in three objects exhibiting absorption. The spectra are centered on H[$\alpha$]{}. H[$\alpha$]{}  sky contamination is marked in Object 00 and 00. Theoretical profiles are from [*kurucz.harvard.edu*]{} for \[Fe/H\]=$-$0.0, [*log g*]{} values of 0.0 $-$0.0, and broadened by a Gaussian to simulate rotation. The profiles suggest values of [*v sin i*]{} in excess of 00 [km s$^{-0}$]{} and ranging to $\sim$ 000 [km s$^{-0}$]{}. Approximate upper and lower limits of velocities are shown. Object 00 and Object 00, exhibiting deep narrow H[$\alpha$]{} are considered to be slow rotators as compared to Object 00. [*Panel d:*]{} Models of the relative central depth of H[$\alpha$]{} ($R_{c+0}$) as compared to model fits in panels [*a, b,*]{} and [*c*]{} are denoted by red squares. The measured values of $R_{c+0}$ for the targets are marked by black circles.](fig0