Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-06-11
Chin.J.Astron.Astrophys. 2 (2001) 533-538
Astronomy and Astrophysics
Astrophysics
submitted, or at http://vega.bac.pku.edu.cn/~rxxu/publications/index_P.htm
Scientific paper
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.
Qiao Guo Jun
Wang Hong-Guang
Xu Ren Xin
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