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<rdf:Description rdf:about="https://catalogues.royalsociety.org:443/CalmView/record/catalog/TG/1/10/58" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/">
  <dc:title>Letter from Thomas gold to Mr Stephen Turk, Space Science adn Astrophysics, Institute for Plasma Research, Stanford University, Via Crespi, Stanford, California</dc:title>
  <dc:description>Encloses the latest version of the histogram of pulsar periods. Asks if he would suggest a good significance test for a bi-model distribution. Would be very important, suggesting that there is a class of pulsars tyhat are set up initially with slow rotation.</dc:description>
  <dc:date>21 February 1973</dc:date>
</rdf:Description>