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            <name>Title</name>
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                <text>Articles</text>
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    <name>Article</name>
    <description>Faculty Publications -Articles</description>
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      <name>Dublin Core</name>
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          <name>Title</name>
          <description>A name given to the resource</description>
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              <text>European VLBI Network observations of the peculiar radio source 4C 35.06 overlapping with a compact group of nine galaxies</text>
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        <element elementId="49">
          <name>Subject</name>
          <description>The topic of the resource</description>
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            <elementText elementTextId="81407">
              <text>galaxies: active; galaxies: clusters: general; galaxies: formation; galaxies: jets; galaxies: nuclei; radio continuum: galaxies</text>
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          <name>Description</name>
          <description>An account of the resource</description>
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              <text>Context. According to the hierarchical structure formation model, brightest cluster galaxies (BCGs) evolve into the most luminous and massive galaxies in the Universe through multiple merger events. The peculiar radio source 4C 35.06 is located at the core of the galaxy cluster Abell 407, overlapping with a compact group of nine galaxies. Low-frequency radio observations have revealed a helical, steep-spectrum, kiloparsec-scale jet structure and inner lobes with less steep spectra, compatible with a recurring active galactic nucleus (AGN) activity scenario. However, the host galaxy of the AGN responsible for the detected radio emission remained unclear. Aims. We aim to identify the host of 4C 35.06 by studying the object at high angular resolution and thereby confirm the recurrent AGN activity scenario. Methods. To reveal the host of the radio source, we carried out very long baseline interferometry (VLBI) observations with the European VLBI Network of the nine galaxies in the group at 1.7 and 4.9 GHz. Results. We detected compact radio emission from an AGN located between the two inner lobes at both observing frequencies. In addition, we detected another galaxy at 1.7 GHz, whose position appears more consistent with the principal jet axis and is located closer to the low-frequency radio peak of 4C 35.06. The presence of another radio-loud AGN in the nonet sheds new light on the BCG formation and provides an alternative scenario in which not just one but two AGNs are responsible for the complex large-scale radio structure.  The Authors 2024.</text>
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          <name>Creator</name>
          <description>An entity primarily responsible for making the resource</description>
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              <text>Veres P.M.; Gabyi K.; Frey S.; Paragi Z.; An T.; Bagchi J.; Bogd ; Biju K.G.; Kun E.; Jacob J.; Adebahr B.</text>
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          <name>Source</name>
          <description>A related resource from which the described resource is derived</description>
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              <text>Astronomy and Astrophysics, Vol-684</text>
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          <name>Publisher</name>
          <description>An entity responsible for making the resource available</description>
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              <text>EDP Sciences</text>
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          <name>Date</name>
          <description>A point or period of time associated with an event in the lifecycle of the resource</description>
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            <elementText elementTextId="81412">
              <text>2024-01-01</text>
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          <name>Identifier</name>
          <description>An unambiguous reference to the resource within a given context</description>
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              <text>&lt;a href="https://doi.org/10.1051/0004-6361/202348729" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1051/0004-6361/202348729&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85191577744&amp;amp;doi=10.1051%2F0004-6361%2F202348729&amp;amp;partnerID=40&amp;amp;md5=2c617e544e2d00b780d31e30d42d9e90" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85191577744&amp;amp;doi=10.1051%2f0004-6361%2f202348729&amp;amp;partnerID=40&amp;amp;md5=2c617e544e2d00b780d31e30d42d9e90&lt;/a&gt;</text>
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          <name>Rights</name>
          <description>Information about rights held in and over the resource</description>
          <elementTextContainer>
            <elementText elementTextId="81414">
              <text>All Open Access; Green Open Access; Hybrid Gold Open Access</text>
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          <name>Relation</name>
          <description>A related resource</description>
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            <elementText elementTextId="81415">
              <text>ISSN: 46361; CODEN: AAEJA</text>
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          <name>Format</name>
          <description>The file format, physical medium, or dimensions of the resource</description>
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            <elementText elementTextId="81416">
              <text>Online</text>
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          <name>Language</name>
          <description>A language of the resource</description>
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            <elementText elementTextId="81417">
              <text>English</text>
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          </elementTextContainer>
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        <element elementId="51">
          <name>Type</name>
          <description>The nature or genre of the resource</description>
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            <elementText elementTextId="81418">
              <text>Article</text>
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          <name>Coverage</name>
          <description>The spatial or temporal topic of the resource, the spatial applicability of the resource, or the jurisdiction under which the resource is relevant</description>
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              <text>Veres P.M., Astronomisches Institut, Ruhr-Universit Bochum, Universitsstr. 150, Bochum, 44801, Germany, Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Konkoly Thege Mikl  15-17, Budapest, 1121, Hungary, CSFK, MTA Centre of Excellence, Konkoly Thege Mikl  15-17, Budapest, 1121, Hungary; Gabyi K., Department of Astronomy, Institute of Physics and Astronomy, ELTE Ev Lord University, Pmy Per sy 1/A, Budapest, 1117, Hungary, HUN-RENELTE Extragalactic Astrophysics Research Group, ELTE Ev Lord University, Pmy Per sy 1/A, Budapest, 1117, Hungary, Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Konkoly Thege Mikl  15-17, Budapest, 1121, Hungary, CSFK, MTA Centre of Excellence, Konkoly Thege Mikl  15-17, Budapest, 1121, Hungary; Frey S., Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Konkoly Thege Mikl  15-17, Budapest, 1121, Hungary, CSFK, MTA Centre of Excellence, Konkoly Thege Mikl  15-17, Budapest, 1121, Hungary, Institute of Physics and Astronomy, ELTE Ev Lord University, Pmy Per sy 1/A, Budapest, 1117, Hungary; Paragi Z., Joint Institute for VLBI ERIC, Oude Hoogeveensedijk 4, Dwingeloo, 7991 PD, Netherlands; An T., Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China, Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing, 100101, China; Bagchi J., Department of Physics and Electronics, CHRIST (Deemed to be University, Hosur Road, Bangalore, 560029, India; Bogd , Center for Astrophysics, Harvard and Smithsonian, 60 Garden Street, Cambridge, 02138, MA, United States; Biju K.G., W.M.O. Arts and Science College, Muttil, Kerala, Wayanad, 673122, India; Kun E., Astronomisches Institut, Ruhr-Universit Bochum, Universitsstr. 150, Bochum, 44801, Germany, Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Konkoly Thege Mikl  15-17, Budapest, 1121, Hungary, CSFK, MTA Centre of Excellence, Konkoly Thege Mikl  15-17, Budapest, 1121, Hungary, Theoretical Physics IV, Faculty for Physics and Astronomy, Ruhr University Bochum, Universitsstr. 150, Bochum, 44780, Germany, Ruhr Astroparticle And Plasma Physics Center, Ruhr-Universit Bochum, Universitsstr. 150, Bochum, 44780, Germany; Jacob J., Newman College, Kerala, Thodupuzha, 685584, India; Adebahr B., Astronomisches Institut, Ruhr-Universit Bochum, Universitsstr. 150, Bochum, 44801, Germany</text>
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