Complexes of the type [Au-2(mu-PP3)(2)]X-2 [X = Cl (1), Br (2), I (3)], [Ag-2(mu-PP3)(2)](NO3)(2) (4), Ag(PP3)Cl (5), M-3(mu-PP3)X-3 [M = Au, X = Cl (10), Br (11), I (12); M = Ag, X = NO3 (13)] and Au-4(mu-PP3)X-4 [X = Cl (14), Br (15), I (16)] have been prepared by interaction between gold(I) or silver(I) salts and the ligand tris[2-(diphenylphosphino) ethyl] phosphine (PP3) in the appropriate molar ratio. Microanalysis, mass spectrometry, IR and NMR spectroscopies and conductivity measurements were used for characterization. 1-3 and 4 are ionic dinuclear species containing four-coordinate gold(I) and four/three coordinate silver(I), respectively. Solutions of 10-12 behave as mixtures of complexes in a 2: 1 [Au-2(mu-PP3)X-2; X = Cl(6), Br(7), I(8)] and 4: 1 (14-16) metal to ligand ratio. 13 and 15 react with free PP3 in solution to generate the ionic compounds 4 and 2, respectively. Complexes 15 and 16, with four linear PAuX fragments per molecule, were shown by X-ray diffraction to consist of dimeric aggregates via close intermolecular gold(I)center dot center dot center dot gold(I) contacts of 3.270 angstrom (15) and 3.184 angstrom (16). The resultant octanuclear systems have an inversion center with two symmetry-related gold(I) atoms being totally out of the aurophilic area and represent a new form of aggregation compared to that found in other halo complexes of gold(I) containing polyphosphines. The luminescence properties of the ligand and complexes, in the solid state, have been studied. Most of the gold systems display intense luminescent emission at room and low temperature. The influence of the halogen on the aurophilic contacts of compounds with a 4: 1 metal to ligand ratio results in different photophysical properties, while 15 and 16 are luminescent complex 14 is nonemissive. The luminescence increases with increasing the phosphine/metal ratio affording for complexes 1-3, without aurophilic contacts, the stronger emissions. Silver complexes 4 and 5 are nonemissive at room temperature and show weaker emissions than gold(I) species at 77 K.