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Article overview
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How fast could a proto-pulsar rotate? | | R.X. Xu
; H.G. Wang
; G.J. Qiao
; | | Date: |
11 Jun 2002 | | Journal: | Chin.J.Astron.Astrophys. 2 (2001) 533-538 | | Subject: | astro-ph | | Affiliation: | PKU), H.G. Wang (PKU), G.J. Qiao (PKU | | 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. | | Source: | arXiv, astro-ph/0206166 | | Services: | Forum | Review | PDF | Favorites | |
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