Heartbeats of a neutron star

Robert V. Wagoner ()
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Robert V. Wagoner: Stanford University

Nature, 2003, vol. 424, issue 6944, 27-28

Abstract: Different oscillations in the flux of X-rays emitted from a neutron star now seem to be linked to the frequency at which the star is spinning. That spin rate in turn hints at what the interior of such a star is made of.

Date: 2003
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DOI: 10.1038/424027a

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