<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-06-27T01:06:43Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/49601" metadataPrefix="mods">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/49601</identifier><datestamp>2023-08-26T05:58:32Z</datestamp><setSpec>com_20.500.14352_14</setSpec><setSpec>col_20.500.14352_15</setSpec></header><metadata><mods:mods xmlns:mods="http://www.loc.gov/mods/v3" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.loc.gov/mods/v3 http://www.loc.gov/standards/mods/v3/mods-3-1.xsd">
   <mods:name>
      <mods:namePart>Orejana García, David</mods:namePart>
   </mods:name>
   <mods:name>
      <mods:namePart>Villaseca González, Carlos</mods:namePart>
   </mods:name>
   <mods:extension>
      <mods:dateAvailable encoding="iso8601">2023-06-20T09:27:33Z</mods:dateAvailable>
   </mods:extension>
   <mods:extension>
      <mods:dateAccessioned encoding="iso8601">2023-06-20T09:27:33Z</mods:dateAccessioned>
   </mods:extension>
   <mods:originInfo>
      <mods:dateIssued encoding="iso8601">2008</mods:dateIssued>
   </mods:originInfo>
   <mods:identifier type="issn">0305-8719</mods:identifier>
   <mods:identifier type="doi">10.1144/SP293.6</mods:identifier>
   <mods:identifier type="uri">https://hdl.handle.net/20.500.14352/49601</mods:identifier>
   <mods:identifier type="officialurl">http://www.geolsoc.org.uk/gsl/op/%3C/publications/books/sp</mods:identifier>
   <mods:abstract>The alkaline lamprophyres and diabases from the Spanish Central System carry a
heterogeneous suite of xenoliths including a group of highly altered ultramafic pyroxenites that
contain Cr–Mg-rich high-T hydrous minerals (Ti-phlogopite and pargasitic to kaersutitic amphibole),
indicative of modal metasomatism. The trace element mineral compositions of these xenoliths
show three patterns: type A xenoliths, with light rare earth element enriched clinopyroxenes
with high field strength element (HFSE) negative anomalies; type B xenoliths, with clinopyroxenes
and amphiboles with high incompatible trace element contents (large ion lithophile elements
(LILE), HFSE and REE); type C xenoliths, with relatively REE- and HFSE-poor clinopyroxenes
and amphiboles. These metasomatic signatures suggest the involvement of three different metasomatic
agents: carbonate, silicate and hydrous fluids or melts, respectively. These agents could
have been derived from the progressive differentiation of a CO2–H2O-rich highly alkaline magma,
genetically related to the Late Permian alkaline magmatism. Because of the original sub-alkaline
nature of the pyroxenite xenoliths, theymight have been formed originally as pyroxene-rich cumulates
associated with underplated Hercynian calc-alkaline basic magmas. Metasomatism as a result of
the infiltration of alkalinemagmaswithin these cumulatesmight explain the relatively high radiogenic
Nd composition of the altered ultramafic xenoliths.</mods:abstract>
   <mods:language>
      <mods:languageTerm>eng</mods:languageTerm>
   </mods:language>
   <mods:accessCondition type="useAndReproduction">open access</mods:accessCondition>
   <mods:titleInfo>
      <mods:title>Heterogeneous metasomatism in cumulate xenoliths from the
Spanish Central System: implications for percolative fractional
crystallization of lamprophyric melts</mods:title>
   </mods:titleInfo>
   <mods:genre>journal article</mods:genre>
</mods:mods></metadata></record></GetRecord></OAI-PMH>