<?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>2026-06-27T12:24:10Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/50065" metadataPrefix="mods">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/50065</identifier><datestamp>2025-10-07T16:37:22Z</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>Gómez De Castro, Ana Inés</mods:namePart>
   </mods:name>
   <mods:name>
      <mods:namePart>Antonicci, A.</mods:namePart>
   </mods:name>
   <mods:extension>
      <mods:dateAvailable encoding="iso8601">2023-06-20T09:37:42Z</mods:dateAvailable>
   </mods:extension>
   <mods:extension>
      <mods:dateAccessioned encoding="iso8601">2023-06-20T09:37:42Z</mods:dateAccessioned>
   </mods:extension>
   <mods:originInfo>
      <mods:dateIssued encoding="iso8601">2006</mods:dateIssued>
   </mods:originInfo>
   <mods:identifier type="citation">Gómez De Castro, A. I., &amp; Antonicci, A. «On the Excitation of the Fe K α Line in AGNs by the Impact of Beams of Highly Relativistic Electrons on the Disk». Astronomische Nachrichten, vol. 327, n.o 10, diciembre de 2006, pp. 989-92. https://doi.org/10.1002/asna.200610678.</mods:identifier>
   <mods:identifier type="issn">0004-6337</mods:identifier>
   <mods:identifier type="doi">10.1002/asna.200610678</mods:identifier>
   <mods:identifier type="uri">https://hdl.handle.net/20.500.14352/50065</mods:identifier>
   <mods:identifier type="officialurl">https://doi.org/10.1002/asna.200610678</mods:identifier>
   <mods:abstract>The propagation of highly relativistic electron beams in dense matter induces a cascade of secondary particles that spreads in the environment redistributing efficiently the beam energy in the medium. Such a highly relativistic beams are expected to be produced in the magnetic reconnection events associated with the flaring activity of the magnetized accretion disks of the AGNs. This contribution presents a quantitative analysis of the possible role of these beams in the excitation of the Fe K alpha line.</mods:abstract>
   <mods:accessCondition type="useAndReproduction">metadata only access</mods:accessCondition>
   <mods:titleInfo>
      <mods:title>On the excitation of the FeK alpha line in AGNs by the impact of beams of highly relativistic electrons on the disk</mods:title>
   </mods:titleInfo>
   <mods:genre>journal article</mods:genre>
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