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b3s
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http://www.w3.org/2002/07/owl#
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oplweb
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webisadb.webdatacommons.org
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The swirls, eddies, filaments and bays" show the interaction of the outer magnetic fluid with the gas, dust and other stuff left behind by the pulsar's progenitor, the massive star that exploded to produce the pulsar.
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nasa.gov
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isap:87000408
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