PLANETARY CAMERA OBSERVATIONS OF THE DOUBLE NUCLEUS OF M31

V- and I-band HST Planetary Camera images of the great spiral galaxy i n Andromeda, M31, show that its inner nucleus consists of two componen ts separated by 0''.49. The outer isophotes of the nucleus at 1''.4 < r < 3''.0 are elongated, but are concentric with the M31 bulge. The nu clear component with the lower surface brightness, P2, is also coincid ent with the bulge photocenter to approximately 0''.05; we argue that it is at the kinematic center of the galaxy. The brighter nuclear comp onent, P1, is well resolved and corresponds to the nuclear core imaged by Stratoscope II. The central V-band luminosity density for P1 is 5 X 10(4)L. pc-3. P2 is highly elongated and has a shallow cusp. Its cen tral V-band luminosity density is > 2 x 10(4) L. pc-3. The total nucle us cannot be modeled as the superposition of two systems each with ell iptical and concentric isophotes. The dark zone between the two peaks is deep and is either evidence for strong dust absorption or that the nuclear components are steeply truncated in this region. No strong cha nges in the V-I color are observed over the nucleus, however. Thus if dust absorption generates the asymmetric nuclear morphology, the dust grain size must be unusually large or the dust optical depth must be e xtremely high. Alternatively the higher surface brightness, off-center nuclear component P1 may be a separate stellar system. The nuclear ve locity dispersion profiles of Dressler & Richstone [ApJ, 324, 701 (198 8)] and Kormendy [ApJ, 325, 128 (1988)] already show that P1 cannot be a dynamically cold system such as a globular cluster. Requiring P1 to survive destruction by a central black hole in M31 may also lead to l ower limits on its mass-to-light ratio. This hypothesis requires us to be looking at M31 at a special time; however, the lifetime of PI agai nst orbital decay may be substantially longer than naive dynamical fri ction arguments would indicate. Under this picture, we argue that PI i s more likely to be a cannibalized galactic nucleus, possibly having i ts own central black hole.