A theoretical model pulsating neutron stars (pulsars)

Physics

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Scientific paper

Angular momentum and moment-of-inertia considerations peculiar to heavy nuclei when applied to neutron stars predict a highly elongated ellipsoidal object, spinning about a minor axis. Preferential emission off the major-axis ends may account for the observed pulsations.
On leave of absence from the National Chemical Laboratory, Poona-8, INDIA.

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