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How fast could a proto-pulsar rotate?

R. X. Xu·H. G. Wang·G. J. Qiao
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Abstract

According to two estimated relations between the initial period and the dynamo-generated magnetic dipole field of pulsars, we calculate the statistical distributions of pulsar initial periods. It is found that proto-pulsars are very likely to have rotation periods between 20 and 30 ms, and that most of the pulsars rotate initially at a period < 60 ms.

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R. X. Xu, H. G. Wang, G. J. Qiao. 2002-06-11. How fast could a proto-pulsar rotate?. https://doi.org/10.1088/1009-9271%2F2%2F6%2F533

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