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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>SILICON DEPLETION in the INTERSTELLAR MEDIUM</text>
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          <name>Subject</name>
          <description>The topic of the resource</description>
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              <text>dust, extinction; ISM: abundances</text>
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              <text>We report interstellar silicon (Si) depletion and dust-phase column densities of Si along 131 Galactic sight lines using archival observations. The data were corrected for differences in the assumed oscillator strength. This is a much larger sample than previous studies but confirms the majority of results, which state that the depletion of Si is correlated with the average density of hydrogen along the line of sight ( (H) as well as the fraction of hydrogen in molecular form ( f(H2)). We also find that the linear part of the extinction curve is independent of Si depletion. Si depletion is correlated with the bump strength (c3/RV) and the FUV curvature (c4/RV) suggesting that silicon plays a significant role in both the 2175 bump and the FUV rise.  2016. The American Astronomical Society. All rights reserved.</text>
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          <name>Creator</name>
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            <elementText elementTextId="136947">
              <text>Haris U.; Parvathi V.S.; Gudennavar S.B.; Bubbly S.G.; Murthy J.; Sofia U.J.</text>
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          <name>Source</name>
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              <text>Astronomical Journal, Vol-151, No. 6</text>
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          <name>Publisher</name>
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              <text>Institute of Physics Publishing</text>
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          <name>Date</name>
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              <text>2016-01-01</text>
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          <name>Identifier</name>
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              <text>&lt;a href="https://doi.org/10.3847/0004-6256/151/6/143" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.3847/0004-6256/151/6/143&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-84975473709&amp;amp;doi=10.3847%2F0004-6256%2F151%2F6%2F143&amp;amp;partnerID=40&amp;amp;md5=80cddbcd2dfac8586f30df64e8bd03fc" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-84975473709&amp;amp;doi=10.3847%2f0004-6256%2f151%2f6%2f143&amp;amp;partnerID=40&amp;amp;md5=80cddbcd2dfac8586f30df64e8bd03fc&lt;/a&gt;</text>
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          <name>Rights</name>
          <description>Information about rights held in and over the resource</description>
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            <elementText elementTextId="136952">
              <text>All Open Access; Bronze Open Access</text>
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          <name>Relation</name>
          <description>A related resource</description>
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              <text>ISSN: 46256</text>
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          <name>Format</name>
          <description>The file format, physical medium, or dimensions of the resource</description>
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              <text>Online</text>
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          <name>Language</name>
          <description>A language of the resource</description>
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              <text>English</text>
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          <name>Type</name>
          <description>The nature or genre of the resource</description>
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              <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>Haris U., Department of Physics, Christ University, Hosur Road, Bangalore, Karnataka, 560029, India; Parvathi V.S., Department of Physics, St. Joseph's College (Autonomous), Lalbagh Road, Bangalore, 560027, India; Gudennavar S.B., Department of Physics, Christ University, Hosur Road, Bangalore, Karnataka, 560029, India; Bubbly S.G., Department of Physics, Christ University, Hosur Road, Bangalore, Karnataka, 560029, India; Murthy J., Indian Institute of Astrophysics, Koramangala, Bangalore, 560034, India; Sofia U.J., Department of Physics, American University, 4400 Massachusetts Avenue, NW, Washington, 20016, DC, United States</text>
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