Where have all the submillisecond pulsars gone?
The existence of pulsars with spin period below one millisecond is expected, though they have not been detected up to now. Their formation depends on the quantity of matter accreted from the companion which, in turn, is limited by the mechanism of mass ejection from the binary. Mass ejection must be...
| 主要な著者: | , , , , , , , , , , |
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| フォーマット: | Conference item |
| 出版事項: |
2001
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