Final processed ASC/HRC G800L spectra for the 14 program stars. A Kurucz ATLAS9 model with T _eff = 20,000 K is shown near the top of the figure for comparison. Weak Hα and H i Paschen absorption lines may be present in our spectra, although they would be close to the detection limit. All the prominent "bumps and wiggles" seen in the ACS spectra are instrumental in the origin.