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<article xmlns:xlink="http://www.w3.org/1999/xlink/">
  <front>
    <article-meta>
      <title-group>
        <article-title>QCD studies with $e^+ e^-$ annihilation data from 130 to 172 GeV</article-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author">
          <name>
            <surname>Cowan</surname>
            <given-names>G D</given-names>
          </name>
        </contrib>
        <contrib contrib-type="author">
          <name>
            <surname>Gao</surname>
            <given-names>Y</given-names>
          </name>
        </contrib>
        <contrib contrib-type="author">
          <name>
            <surname>Jones</surname>
            <given-names>R</given-names>
          </name>
        </contrib>
        <contrib contrib-type="author">
          <name>
            <surname>Stenzel</surname>
            <given-names>H</given-names>
          </name>
        </contrib>
      </contrib-group>
      <pub-date pub-type="pub">
        <year>1997</year>
      </pub-date>
      <self-uri xlink:href="http://cds.cern.ch/record/407102"/>
      <self-uri xlink:href="http://documents.cern.ch/cgi-bin/setlink?base=preprint&amp;categ=cern&amp;id=open-99-323"/>
      <self-uri xlink:href="http://cds.cern.ch/record/407102/files/open-99-323.pdf"/>
      <self-uri xlink:href="http://cds.cern.ch/record/407102/files/open-99-323.ps.gz"/>
    </article-meta>
    <abstract>Hadronic events produced at LEP at centre-of-mass energies of 130, 136, 161 and 172 GeV have been studied and compared with QCD predictions. Distributions of event-shape observables, jet rates, momentum spectra and multiplicities are presented and compared to the predictions of several Monte Carlo models and analytic QCD calculations. From a fit of O(alpha_s^2)+NLLA QCD calculations to the differential two-jet rate, alpha_s has been determined at various energies. The mean charged particle multiplicities and the peak positions xi_star in the xi = ln(1/x_p) distribution have also been determined. These results have been compared to lower energy data and to analytic QCD or Monte Carlo predictions for their energy evolution.</abstract>
  </front>
  <article-type>PREPRINT</article-type>
</article>

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