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           <title>Stars with Debris Disks and Planets</title>
           <identifier>ivo://svo.cab/debris</identifier>
           <curation>
             <publisher ivo-id="ivo://svo.cab">SVO CAB</publisher>
              <contact>
                 <name>Enrique Solano</name>
                <email>esm@cab.inta-csic.es</email>
              </contact>
           </curation>
           <content>
              <subject>stars</subject>
              <description>Planetary systems are built by planets and planetesimals formed in
        circumstellar disks surrounding young pre-main sequence stars. Once in
        the main-sequence collisions of planetesimals produce small dust
        particles giving rise to the so-called debris disks. The mutual
        interaction among planets, planetesimals and debris disks,  and with
        their host stars determines the fate of planetary systems.

        Currently thousands of main-sequence stars are known to host planets and
        debris disks. The Solar System with its peculiarities is just one of
        such planetary systems. However, only few tens of stars are known to
        host simultaneously both planets and debris disks. Therefore, the
        study of those systems is particularly valuable to widen our knowledge
        of planetary systems and their evolution.

        This page just collects some of the properties of the known, to our knowledge,
         solar-type stars hosting both planets and debris disk.</description>
              <referenceURL>http://svo2.cab.inta-csic.es/vocats/debris2/</referenceURL>
             <contentLevel>Research</contentLevel>
           </content>
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                 <accessURL use="full">http://svo2.cab.inta-csic.es/vocats/debris2/cs.php?</accessURL>
              </interface>
              <verbosity>true</verbosity>
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