The alkaline lamprophyres and diabases of the Spanish Central System carry a heterogeneous suite of xenoliths which includes scarce pyroxenitic and hornblenditic types that can be divided in two groups: (a) pyroxenite xenoliths, including spinel clinopyroxenites and spinel websterites with granoblastic textures, and (b) hornblende-bearing clinopyroxenites and hornblen dites (here after called hornblenditic xenoliths) characterised by the presence of Ti-rich kaersutitic amphibole and magmatic textures, Both groups of xenoliths can be assigned to the Al-augite series of Wilshire and Shervais (1975) xenolith suite has a very homogeneous isotopic composition, close to the isotopically depleted values of high ENd and low 87 Sr/ 86 Sr ratios of one of the pyroxenite xenoliths, Some of these ultramafic xenoliths fall within the isotopic compositional range of their host alkaline dykes, which also define a bipolar compositional field, suggesting that most of them are cogenetic with the lamprophyres, P-T estimates yield temperatures in the range of 970-1 080 °c and pressures mainly from 0,9 to 1,2 GPa for pyroxenites, whilst hornblenditic xenoliths give lower (and probably underestimated) pressures (0,7-0,9 GPa), This pressure range is in agreement with pyroxenites being fonned by an underplating event at the upper mantle-lower crust boundary, whereas pressure estimates for hornblenditic xenoliths suggest equilibration within the lower crust