  We present analyses of the ASCA X-ray spectra of two Seyfert galaxies, Tololo
0109-383 and ESO 138-G1. In both cases, spectral fitting reveals two
statistically acceptable continuum models: Compton reflection and partial
covering. Both spectra have strong iron K-alpha lines, with equivalent widths
greater than 1.5 keV. These large equivalent widths are suggestive of heavier
obscuration than that directly indicated by the partial-covering models
(approximately 2 x 10^23 cm^-2), with the actual column densities being
`Compton-thick' (i.e. N_H > 1.5 x 10^24 cm^-2). We use the hard X-ray/[O III]
flux correlation for Seyferts and data from the literature to provide
additional support for this hypothesis. Since Tololo 0109-383 is known to have
optical type 1 characteristics such as broad Balmer line components and Fe II
emission, this result marks it as a notable object.
