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{"ops":[{"insert":"The period of the crab pulsar is 33 ms and its observed value of T is 1263 years. Assuming the crab neutron star has a radius of 112km, and \ufeff\ufeff\ufeff\ufeffangle where magnetic dipole moment is inclined to the star rotation axis is 90, and a moment of inertia of 10"},{"attributes":{"script":"super"},"insert":"45 "},{"insert":"gcm"},{"attributes":{"script":"super"},"insert":"2"},{"insert":", what is the approximate magnitude of the surface B necessary to account for the observed spin down of the crab pulsar? What is the power radiated?\n"}]}
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