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<adc:VO_Catalog_ADC xmlns:adc="http://adc.astro.umd.edu/dataset_054" xmlns:au="http://adc.astro.umd.edu/Units" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:cat="http://www.ivoa.net/Catalog" xmlns:cha="http://www.ivoa.net/Characterization" xmlns:col="http://www.ivoa.net/Collection" xmlns:stc="http://www.ivoa.net/xml/STC/stc-v1.20" xmlns:r="http://www.ivoa.net/xml/STC/STCregion/v1.20" xmlns:crd="http://www.ivoa.net/xml/STC/STCcoords/v1.20" xmlns:h="http://www.ivoa.net/Provenance" xmlns:p="http://www.ivoa.net/Publications" xmlns:ppl="http://www.ivoa.net/People" xmlns:ucd="http://www.ivoa.net/UCD1+" xmlns:u="http://www.ivoa.net/Units" xmlns:q="http://www.ivoa.net/Quantity" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" cid="adc_1134" name="A New List of Trapezium-Type Multiple Systems" xsi:schemaLocation="http://adc.astro.umd.edu/dataset_054 dataset_054.xsd">
  <dc:identifier>1134</dc:identifier>
  <h:provenance provenanceId="history_1134">
    <h:creation>
      <h:creator>
        <ppl:person>
          <ppl:firstName>Francois</ppl:firstName>
          <ppl:lastName>Ochsenbein</ppl:lastName>
          <ppl:institution>
            <ppl:name>CDS</ppl:name>
          </ppl:institution>
        </ppl:person>
      </h:creator>
      <stc:date>1997-02-11</stc:date>
      <h:acknowledgement>The author is thankful to professor V.A.Ambartsumian for valuable advices during the compilation of the catalogue of trapezium-type multiple systems, and also to the collaborators of the Abastumani Astrophysical Observatory M.Butikashvili and N.Kiselyova for the transfer of the trapezia catalogue on the magnetic tape. Author's address: G.N.Salukvadze Astrophysical Observatory 383762 Abastumani, Georgia</h:acknowledgement>
    </h:creation>
    <h:revisions>
      <h:revision>
        <h:revisor>
          <ppl:team>
            <ppl:name>ADC staff</ppl:name>
            <ppl:institution>
              <ppl:name>ADC</ppl:name>
              <ppl:address>
                <ppl:street>Code 630, Goddard Space Flight Center/NASA</ppl:street>
                <ppl:postcode>20771</ppl:postcode>
                <ppl:city>Greenbelt</ppl:city>
                <ppl:state>Maryland</ppl:state>
                <ppl:country>United States of America</ppl:country>
              </ppl:address>
            </ppl:institution>
          </ppl:team>
          <p:note><![CDATA[Revision using version 1.36 of ADC's legacy conversion pipeline]]></p:note>
        </h:revisor>
        <stc:date>2002-07-12</stc:date>
        <p:note><![CDATA[XML generated from CDS/ADC ReadMe document and associated data files using txt2ML Rules Set: 1.56]]></p:note>
      </h:revision>
      <h:revision>
        <h:revisor>
          <ppl:team>
            <ppl:name>UMd-ADC staff</ppl:name>
            <ppl:institution>
              <ppl:name>UMd Astronomical Data Center</ppl:name>
              <ppl:address>
                <ppl:street>Department of Astronomy, University of Maryland</ppl:street>
                <ppl:postcode>20742</ppl:postcode>
                <ppl:city>College Park</ppl:city>
                <ppl:state>Maryland</ppl:state>
                <ppl:country>United States of America</ppl:country>
              </ppl:address>
              <ppl:email>thomas@astro.umd.edu</ppl:email>
              <ppl:url>http://archive.astro.umd.edu/archive</ppl:url>
            </ppl:institution>
          </ppl:team>
          <p:note><![CDATA[Revision using version 0.16 of the quantity/dataset transform pipeline.]]></p:note>
        </h:revisor>
        <stc:date>2005-09-30T05:02:58-04:00</stc:date>
        <p:note><![CDATA[This version of the document has unverified coordinate system information. Use at your ownrisk!]]></p:note>
      </h:revision>
    </h:revisions>
  </h:provenance>
  <p:references referencesId="ref_1134">
    <p:reference referenceId="srf1" type="source">
      <dc:title>A New List of Trapezium-Type Multiple Systems</dc:title>
      <p:abstract>
        <p:para><![CDATA[
    The present catalogue of Trapezium-type Multiple Systems was compiled
    on the basis of the Index Catalogue of Visual Binary Stars (IDS,
    Jeffers et al., 1963).]]></p:para>
        <p:para><![CDATA[    At the period of compilation of the Abastumani catalogue, IDS was the
    most complete catalogue concerning not only stars, but also the data
    on double stars. Besides giving relative positions, IDS presents the
    coordinates at 1900 and 2000 epochs, as well as in most cases
    magnitudes, spectral classes and proper motions. IDS contains all
    double and multiple stars from the North to the South poles with
    relative positions published up to the end of 1960, their total number
    being 64247.]]></p:para>
        <p:para><![CDATA[    In order to select optimum value of K (ratio of the largest to the
    smallest distances among the components), which is the main criterion
    for relating a multiple star to the trapezium type, the dependence of
    the observed trapezia number on the K value has been analysed, and the
    value 2.6 adopted for it. To exclude optical components, upper limits
    for the distances of faint components to the main star have been
    introduced, and the components fainter than 12.5mag were excluded
    altogether (Salukvadze, 1978).]]></p:para>
        <p:para><![CDATA[    The catalogue of Trapezium-type Multiple Systems contains 412
    trapezia, for which, after examining all main spectral catalogues
    (Jaschek et al., 1964; Kennedy et al., 1974; Houck et al.,
    1975; Cruz-Gonzales et al., 1974; Lindsey et al., 1968), spectral
    classes in the MK system have been specified. This was done for 100
    systems, including 65 stars of O and B spectral classes.]]></p:para>
        <p:para><![CDATA[    The following data on trapezia are given in the catalogue: positional
    angles and distances, magnitudes and spectral classes according to HD
    as well as MK, the ADS and BD identification number of the main star.]]></p:para>
        <p:para><![CDATA[    On the basis of the probability, deduced by Ambartsumian (1954), the
    number of pseudo-trapezia was estimated, that is, the number of
    multiple stars, which in fact have no trapezium-type configurations,
    but are observed as trapezia as a result of their projection on the
    celestial sphere. The number of estimated pseudo-trapezia is 167. It
    should be mentioned that among 59 trapezia, the main components of
    which are of the O-B2 spectral class, there are only 5
    pseudo-trapezia. This enables us to maintain that there is a
    considerable percent of real trapezia among the ones of mentioned
    spectral classes.]]></p:para>
        <p:para><![CDATA[    Evaluation of the number of optical systems, formed as a result of the
    appearance of background stars in circles, which are
    determined by the upper limits of components' distances, led to their
    insignificant number 9.]]></p:para>
      </p:abstract>
      <p:description/>
      <p:author>
        <ppl:person>
          <ppl:initial>G</ppl:initial>
          <ppl:initial>N</ppl:initial>
          <ppl:lastName>Salukvadze</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:other>
        <p:name>Byull. Abastumani Astrofiz. Obs. No. 49, pp. 39-68</p:name>
        <stc:date>1978-??-??</stc:date>
        <p:bibcode>1978AbaOB..49...39S</p:bibcode>
      </p:other>
    </p:reference>
    <p:reference referenceId="srf2" type="source">
      <dc:title>The Catalogue of Trapezium-Type Multiple Systems</dc:title>
      <p:abstract>
        <p:para><![CDATA[
    The present catalogue of Trapezium-type Multiple Systems was compiled
    on the basis of the Index Catalogue of Visual Binary Stars (IDS,
    Jeffers et al., 1963).]]></p:para>
        <p:para><![CDATA[    At the period of compilation of the Abastumani catalogue, IDS was the
    most complete catalogue concerning not only stars, but also the data
    on double stars. Besides giving relative positions, IDS presents the
    coordinates at 1900 and 2000 epochs, as well as in most cases
    magnitudes, spectral classes and proper motions. IDS contains all
    double and multiple stars from the North to the South poles with
    relative positions published up to the end of 1960, their total number
    being 64247.]]></p:para>
        <p:para><![CDATA[    In order to select optimum value of K (ratio of the largest to the
    smallest distances among the components), which is the main criterion
    for relating a multiple star to the trapezium type, the dependence of
    the observed trapezia number on the K value has been analysed, and the
    value 2.6 adopted for it. To exclude optical components, upper limits
    for the distances of faint components to the main star have been
    introduced, and the components fainter than 12.5mag were excluded
    altogether (Salukvadze, 1978).]]></p:para>
        <p:para><![CDATA[    The catalogue of Trapezium-type Multiple Systems contains 412
    trapezia, for which, after examining all main spectral catalogues
    (Jaschek et al., 1964; Kennedy et al., 1974; Houck et al.,
    1975; Cruz-Gonzales et al., 1974; Lindsey et al., 1968), spectral
    classes in the MK system have been specified. This was done for 100
    systems, including 65 stars of O and B spectral classes.]]></p:para>
        <p:para><![CDATA[    The following data on trapezia are given in the catalogue: positional
    angles and distances, magnitudes and spectral classes according to HD
    as well as MK, the ADS and BD identification number of the main star.]]></p:para>
        <p:para><![CDATA[    On the basis of the probability, deduced by Ambartsumian (1954), the
    number of pseudo-trapezia was estimated, that is, the number of
    multiple stars, which in fact have no trapezium-type configurations,
    but are observed as trapezia as a result of their projection on the
    celestial sphere. The number of estimated pseudo-trapezia is 167. It
    should be mentioned that among 59 trapezia, the main components of
    which are of the O-B2 spectral class, there are only 5
    pseudo-trapezia. This enables us to maintain that there is a
    considerable percent of real trapezia among the ones of mentioned
    spectral classes.]]></p:para>
        <p:para><![CDATA[    Evaluation of the number of optical systems, formed as a result of the
    appearance of background stars in circles, which are
    determined by the upper limits of components' distances, led to their
    insignificant number 9.]]></p:para>
      </p:abstract>
      <p:description/>
      <p:author>
        <ppl:person>
          <ppl:initial>G</ppl:initial>
          <ppl:initial>N</ppl:initial>
          <ppl:lastName>Salukvadze</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:journal>
        <p:name>Astrofizika</p:name>
        <p:volume>14</p:volume>
        <p:pageno>57</p:pageno>
        <stc:date>1978-??-??</stc:date>
        <p:bibcode>1978Afz....14...57S</p:bibcode>
      </p:journal>
    </p:reference>
    <adc:reference referenceId="seeAlso_1_1" type="seeAlso">
      <dc:title>The Washington Visual Double Star Catalog (Continuation of the IDS)</dc:title>
      <p:author>
        <ppl:person>
          <ppl:lastName>Continuation</ppl:lastName>
        </ppl:person>
      </p:author>
      <adc:holding role="similar">I/237: The Washington Visual Double Star Catalog (Continuation of the IDS)<adc:altname namespace="http://adc.astro.umd.edu">1237</adc:altname>
</adc:holding>
    </adc:reference>
    <p:reference referenceId="rrf1" type="related">
      <p:author>
        <ppl:person>
          <ppl:initial>V</ppl:initial>
          <ppl:initial>A</ppl:initial>
          <ppl:lastName>Ambartsumian</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:journal>
        <p:name>Com. Byurakan Obs.</p:name>
        <p:volume>13</p:volume>
        <p:pageno>1-35</p:pageno>
        <stc:date>1954-??-??</stc:date>
      </p:journal>
    </p:reference>
    <p:reference referenceId="rrf2" type="related">
      <dc:title>A catalogue of galactic O stars. The ionization of the low density interstellar medium by runaway stars.</dc:title>
      <p:author>
        <ppl:person>
          <ppl:initial>C</ppl:initial>
          <ppl:lastName>Cruz-Gonzalez</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:author>
        <ppl:person>
          <ppl:initial>E</ppl:initial>
          <ppl:lastName>Recillas-Cruz</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:author>
        <ppl:person>
          <ppl:initial>R</ppl:initial>
          <ppl:lastName>Costero</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:author>
        <ppl:person>
          <ppl:initial>M</ppl:initial>
          <ppl:lastName>Peimbert</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:author>
        <ppl:person>
          <ppl:initial>S</ppl:initial>
          <ppl:lastName>Torres-Peimbeert</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:journal>
        <p:name>Revista Mexicana de Astronomia y Astrofisica</p:name>
        <p:volume>1</p:volume>
        <p:pageno>211</p:pageno>
        <stc:date>1974-??-??</stc:date>
        <p:bibcode>1974RMxAA...1..211C</p:bibcode>
      </p:journal>
    </p:reference>
    <p:reference referenceId="rrf3" type="related">
      <dc:title>Michigan Catalogue of two-dimensional spectral types for the HD star</dc:title>
      <p:author>
        <ppl:person>
          <ppl:firstName>Nancy</ppl:firstName>
          <ppl:lastName>Houk</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:author>
        <ppl:person>
          <ppl:firstName>Anne</ppl:firstName>
          <ppl:initial>P</ppl:initial>
          <ppl:lastName>Cowley</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:book>
        <p:publisher>Department of Astronomy, University of Michigan</p:publisher>
        <p:city>Ann Arbor</p:city>
        <stc:date>1975-??-??</stc:date>
      </p:book>
    </p:reference>
    <p:reference referenceId="rrf4" type="related">
      <dc:title>Catalogue of stellar spectra classified in the Morgan-Keenan system</dc:title>
      <p:author>
        <ppl:person>
          <ppl:firstName>Carlos</ppl:firstName>
          <ppl:lastName>Jaschek</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:author>
        <ppl:person>
          <ppl:firstName>Horacio</ppl:firstName>
          <ppl:lastName>Conde</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:author>
        <ppl:person>
          <ppl:prefix>de</ppl:prefix>
          <ppl:firstName>Amelia</ppl:firstName>
          <ppl:initial>C</ppl:initial>
          <ppl:lastName>Sierra</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:journal>
        <p:name>Observatory Astronomical La Plata Series Astronomies</p:name>
        <p:volume>28</p:volume>
        <p:pageno>1</p:pageno>
        <stc:date>1964-??-??</stc:date>
        <p:bibcode>1964PLPla..28....1J</p:bibcode>
      </p:journal>
    </p:reference>
    <p:reference referenceId="rrf5" type="related">
      <dc:title>Index catalogue of visual double stars, 1961.0</dc:title>
      <p:author>
        <ppl:person>
          <ppl:firstName>Hamilton</ppl:firstName>
          <ppl:initial>M</ppl:initial>
          <ppl:lastName>Jeffers</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:author>
        <ppl:person>
          <ppl:prefix>van</ppl:prefix>
          <ppl:firstName>Willem</ppl:firstName>
          <ppl:initial>H</ppl:initial>
          <ppl:lastName>Denbos</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:author>
        <ppl:person>
          <ppl:firstName>Frances</ppl:firstName>
          <ppl:initial>M</ppl:initial>
          <ppl:lastName>Greeby</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:book>
        <p:publisher>University of California</p:publisher>
        <p:city>Mount Hamilton</p:city>
        <stc:date>1963-??-??</stc:date>
      </p:book>
    </p:reference>
    <p:reference referenceId="rrf6" type="related">
      <dc:title>MK spectral classifications, published since Jaschek's La Plata Catalogue</dc:title>
      <p:author>
        <ppl:person>
          <ppl:firstName>Pamela</ppl:firstName>
          <ppl:initial>M</ppl:initial>
          <ppl:lastName>Kennedy</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:author>
        <ppl:person>
          <ppl:firstName>William</ppl:firstName>
          <ppl:lastName>Buscombe</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:book>
        <p:publisher>Northwestern University</p:publisher>
        <p:city>Evanston</p:city>
        <stc:date>1974-??-??</stc:date>
      </p:book>
    </p:reference>
    <p:reference referenceId="rrf7" type="related">
      <dc:title>A revised spectral classification system and a new catalogue for galactic Wolf-Rayet stars</dc:title>
      <p:author>
        <ppl:person>
          <ppl:firstName>Lindsey</ppl:firstName>
          <ppl:initial>F</ppl:initial>
          <ppl:lastName>Smith</ppl:lastName>
        </ppl:person>
      </p:author>
      <p:journal>
        <p:name>Monthly Notices of the RAS</p:name>
        <p:volume>138</p:volume>
        <p:pageno>109</p:pageno>
        <stc:date>1968-??-??</stc:date>
        <p:bibcode>1968MNRAS.138..109S</p:bibcode>
      </p:journal>
    </p:reference>
  </p:references>
  <adc:data>
    <cat:VOCatalog cid="adc_cat_data" name="data" description="The Catalogue of Trapezium Multiple Systems">
      <dc:identifier>1134_data</dc:identifier>
      <h:refProvenance provenanceIdRef="history_1134"/>
      <p:refReferences referencesIdRef="ref_1134"/>
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          </col:property>
          <col:property name="SpType1" description="Spectral class of the main star in the MK system (1)" qid="data_SpType1">
            <cha:limits>
              <q:refQuantity qidRef="data_SpType1"/>
              <cha:min/>
              <cha:max/>
            </cha:limits>
            <q:axes>
              <q:refQuantity qidRef="obj_data"/>
            </q:axes>
            <u:unitless/>
            <q:string width="11" noDataValue="           "/>
            <q:values fromResource="res_data"/>
          </col:property>
          <col:property name="ADS" description="? ADS number (1)" qid="data_ADS">
            <cha:limits>
              <q:refQuantity qidRef="data_ADS"/>
              <cha:min>202</cha:min>
              <cha:max>17032</cha:max>
            </cha:limits>
            <q:axes>
              <q:refQuantity qidRef="obj_data"/>
            </q:axes>
            <u:unitless/>
            <q:integer noDataValue="-9999" width="5" type="decimal"/>
            <q:values fromResource="res_data"/>
          </col:property>
          <col:property name="DM" description="Durchmusterung number (1)" qid="data_DM">
            <cha:limits>
              <q:refQuantity qidRef="data_DM"/>
              <cha:min/>
              <cha:max/>
            </cha:limits>
            <q:axes>
              <q:refQuantity qidRef="obj_data"/>
            </q:axes>
            <u:unitless/>
            <q:string width="9" noDataValue="         "/>
            <q:values fromResource="res_data"/>
          </col:property>
        </col:object>
      </cat:data>
    </cat:VOCatalog>
  </adc:data>
</adc:VO_Catalog_ADC>
