  We compare a deep (37 ks) Chandra ACIS-S image of the M31 bulge to Local
Group Survey narrow-band optical data and Very Large Array (VLA) radio data of
the same region. Our precisely registered images reveal two new optical shells
with X-ray counterparts. These shells have sizes, [S II]/H-alpha flux ratios,
and X-ray spectral properties typical of supernova remnants (SNRs) with ages of
9$^{+3}_{-4}$ and 17$^{+6}_{-9}$ kyr. Analysis of complementary VLA data
reveals the radio counterparts, further confirming that they are SNRs. We
discuss and compare the properties and morphologies of these SNRs at the
different wavelengths.
