A Few Deductions from the Observational Data on Pulsar Braking Index
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概要
- 論文の詳細を見る
Observationally derived values for the braking index of three pulsars are used to infer the effective radius at which the angular momentum loss is taking place. The results indicate that this radius is well within the light cylinder, and that the wind and magnetospheric structures may be quite different from those given in the standard model by Goldreich and Julian. A new picture which could take the place of the current views is proposed.Radio pulsarsbraking indexpulsar winds
- 東北大学の論文
- 1991-01-31
著者
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KUDOH Takahiro
Astronomical Data Analysis Center, National Astronomical Observatory
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Kudoh T
Astronomical Institute Faculty Of Science Tohoku University
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Kaburaki Osamu
Astronomical Institute Faculty Of Science Tohoku University
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