<?xml version="1.0" encoding="UTF-8"?>
<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns="http://purl.org/rss/1.0/" xmlns:taxo="http://purl.org/rss/1.0/modules/taxonomy/" xmlns:sy="http://purl.org/rss/1.0/modules/syndication/" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:rss="http://purl.org/rss/1.0/">
  <channel rdf:about="http://www.edpsciences.org/articles/aa/rss/TOCRSS/rss.xml">
    <title>Recent articles published in 'Astronomy &amp; Astrophysics'</title>
    <link>http://www.aanda.org</link>
    <description>Recent articles published in 'Astronomy &amp; Astrophysics'</description>
    <items>
      <rdf:Seq>
        <rdf:li resource="http://www.aanda.org/10.1051/0004-6361/201321590"/>
        <rdf:li resource="http://www.aanda.org/10.1051/0004-6361/201321431"/>
        <rdf:li resource="http://www.aanda.org/10.1051/0004-6361/201321465"/>
      </rdf:Seq>
    </items>
    <sy:updatePeriod>daily</sy:updatePeriod>
    <sy:updateFrequency>1</sy:updateFrequency>
    <sy:updateBase>2013-05-22T18:11:53Z</sy:updateBase>
    <dc:publisher>EDP Sciences</dc:publisher>
    <dc:rights>Copyright (c) EDP Sciences 2013</dc:rights>
    <prism:copyright>Copyright (c) EDP Sciences 2013</prism:copyright>
    <prism:issn>0004-6361</prism:issn>
    <prism:publicationName>Astronomy &amp; Astrophysics</prism:publicationName>
  </channel>
  <rss:item rdf:about="http://www.aanda.org/10.1051/0004-6361/201321590">
    <rss:title>The influence of magnetic fields, turbulence, and UV radiation on the formation of supermassive black holes</rss:title>
    <rss:link>http://www.aanda.org/10.1051/0004-6361/201321590</rss:link>
    <rss:description>Authors: C. Van Borm and M. Spaans.&lt;br /&gt;Astronomy &amp; Astrophysics Vol. 553 , page L9&lt;br /&gt;Published online: 22/05/2013&lt;br /&gt;
       Keywords:
       early Universe ; black hole physics ; magnetic fields ; turbulence.</rss:description>
    <dc:title>The influence of magnetic fields, turbulence, and UV radiation on the formation of supermassive black holes</dc:title>
    <dc:creator>C. Van Borm</dc:creator>
    <dc:creator>M. Spaans</dc:creator>
    <dc:subject>early Universe</dc:subject>
    <dc:subject>black hole physics</dc:subject>
    <dc:subject>magnetic fields</dc:subject>
    <dc:subject>turbulence</dc:subject>
    <dc:date>2013-05-22</dc:date>
    <dc:format>text/html</dc:format>
    <dc:identifier>10.1051/0004-6361/201321590</dc:identifier>
    <dc:source>Astronomy &amp; Astrophysics  Vol. 553</dc:source>
    <prism:category>abstract</prism:category>
    <prism:issueIdentifier>aa/2013/05</prism:issueIdentifier>
    <prism:publicationDate>2013-05-22</prism:publicationDate>
    <prism:publicationName>Astronomy &amp; Astrophysics</prism:publicationName>
    <prism:startingPage>L9</prism:startingPage>
    <prism:volume>553</prism:volume>
  </rss:item>
  <rss:item rdf:about="http://www.aanda.org/10.1051/0004-6361/201321431">
    <rss:title>Connection between dense gas mass fraction, turbulence driving, and star formation efficiency of molecular clouds⋆</rss:title>
    <rss:link>http://www.aanda.org/10.1051/0004-6361/201321431</rss:link>
    <rss:description>Authors: J. Kainulainen, C. Federrath and T. Henning.&lt;br /&gt;Astronomy &amp; Astrophysics Vol. 553 , page L8&lt;br /&gt;Published online: 17/05/2013&lt;br /&gt;
       Keywords:
       ISM: clouds ; ISM: structure ; stars: formation ; turbulence.</rss:description>
    <dc:title>Connection between dense gas mass fraction, turbulence driving, and star formation efficiency of molecular clouds⋆</dc:title>
    <dc:creator>J. Kainulainen</dc:creator>
    <dc:creator>C. Federrath</dc:creator>
    <dc:creator>T. Henning</dc:creator>
    <dc:subject>ISM: clouds</dc:subject>
    <dc:subject>ISM: structure</dc:subject>
    <dc:subject>stars: formation</dc:subject>
    <dc:subject>turbulence</dc:subject>
    <dc:date>2013-05-17</dc:date>
    <dc:format>text/html</dc:format>
    <dc:identifier>10.1051/0004-6361/201321431</dc:identifier>
    <dc:source>Astronomy &amp; Astrophysics  Vol. 553</dc:source>
    <prism:category>abstract</prism:category>
    <prism:issueIdentifier>aa/2013/05</prism:issueIdentifier>
    <prism:publicationDate>2013-05-17</prism:publicationDate>
    <prism:publicationName>Astronomy &amp; Astrophysics</prism:publicationName>
    <prism:startingPage>L8</prism:startingPage>
    <prism:volume>553</prism:volume>
  </rss:item>
  <rss:item rdf:about="http://www.aanda.org/10.1051/0004-6361/201321465">
    <rss:title>Hi-C and AIA observations of transverse magnetohydrodynamic waves in active regions⋆</rss:title>
    <rss:link>http://www.aanda.org/10.1051/0004-6361/201321465</rss:link>
    <rss:description>Authors: R. J. Morton and J. A. McLaughlin.&lt;br /&gt;Astronomy &amp; Astrophysics Vol. 553 , page L10&lt;br /&gt;Published online: 22/05/2013&lt;br /&gt;
       Keywords:
       Sun: corona ; Sun: chromosphere ; waves ; magnetohydrodynamics (MHD).</rss:description>
    <dc:title>Hi-C and AIA observations of transverse magnetohydrodynamic waves in active regions⋆</dc:title>
    <dc:creator>R. J. Morton</dc:creator>
    <dc:creator>J. A. McLaughlin</dc:creator>
    <dc:subject>Sun: corona</dc:subject>
    <dc:subject>Sun: chromosphere</dc:subject>
    <dc:subject>waves</dc:subject>
    <dc:subject>magnetohydrodynamics (MHD)</dc:subject>
    <dc:date>2013-05-22</dc:date>
    <dc:format>text/html</dc:format>
    <dc:identifier>10.1051/0004-6361/201321465</dc:identifier>
    <dc:source>Astronomy &amp; Astrophysics  Vol. 553</dc:source>
    <prism:category>abstract</prism:category>
    <prism:issueIdentifier>aa/2013/05</prism:issueIdentifier>
    <prism:publicationDate>2013-05-22</prism:publicationDate>
    <prism:publicationName>Astronomy &amp; Astrophysics</prism:publicationName>
    <prism:startingPage>L10</prism:startingPage>
    <prism:volume>553</prism:volume>
  </rss:item>
</rdf:RDF>
