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            <name>Title</name>
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    <name>Article</name>
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          <name>Title</name>
          <description>A name given to the resource</description>
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              <text>Active galactic nucleus feedback in NGC 3982</text>
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          <name>Subject</name>
          <description>The topic of the resource</description>
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              <text>Galaxies: Active; Galaxies: individual: NGC 3982; Galaxies: star formation; Ultraviolet: galaxies</text>
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          <name>Description</name>
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              <text>The energetic feedback from supermassive black holes can influence star formation at the centres of galaxies. Observational evidence for active galactic nucleus (AGN) impact on star formation can be searched for in galaxies by combining ultraviolet imaging and optical integral field unit data. The ultraviolet flux directly traces recent star formation, and the integral field unit data can reveal dust attenuation, gas ionisation mechanisms, and gas kinematics from the central regions of the galaxy disk. A pilot study on NGC 3982 shows star formation suppression in the central regions of the galaxy, likely due to negative AGN feedback, and enhanced star formation in the outer regions. The case of NGC 3982 could be observational evidence of AGN feedback operating in a Seyfert galaxy.   2022 EDP Sciences. All rights reserved.</text>
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        <element elementId="39">
          <name>Creator</name>
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              <text>Joseph P.; George K.; Paul K.T.</text>
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          <name>Source</name>
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              <text>Astronomy and Astrophysics, Vol-667</text>
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          <name>Publisher</name>
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              <text>EDP Sciences</text>
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          <name>Date</name>
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              <text>2022-01-01</text>
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          <name>Identifier</name>
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              <text>&lt;a href="https://doi.org/10.1051/0004-6361/202243923" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1051/0004-6361/202243923&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85144174963&amp;amp;doi=10.1051%2F0004-6361%2F202243923&amp;amp;partnerID=40&amp;amp;md5=4e7a3c3a4bad668d654a1348fbccaccc" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85144174963&amp;amp;doi=10.1051%2f0004-6361%2f202243923&amp;amp;partnerID=40&amp;amp;md5=4e7a3c3a4bad668d654a1348fbccaccc&lt;/a&gt;</text>
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          <name>Rights</name>
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            <elementText elementTextId="104902">
              <text>All Open Access; Green Open Access; Hybrid Gold Open Access</text>
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          <name>Relation</name>
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              <text>ISSN: 46361; CODEN: AAEJA</text>
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              <text>Online</text>
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              <text>English</text>
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              <text>Joseph P., Department of Physics, CHRIST University, Bangalore, 560029, India, Indian Institute of Astrophysics, Bangalore, 560034, India; George K., Faculty of Physics, Ludwig-Maximilians-Universit, Scheinerstr. 1, Munich, 81679, Germany; Paul K.T., Department of Physics, CHRIST University, Bangalore, 560029, India</text>
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