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- W1978732406 abstract "We present an analysis of the spin-down parameters for 131 radio pulsars for which has been well determined. These pulsars have characteristic ages ranging from 103 to 108 yr and spin periods in the range 0.4-30 s; nearly equal numbers of pulsars have as have . We find a strong correlation of with , independent of the sign of. We suggest that this trend can be accounted for by small, stochastic deviations in the spin-down torque that are directly proportional (in magnitude) to the spin-down torque." @default.
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- W1978732406 date "2006-07-01" @default.
- W1978732406 modified "2023-09-27" @default.
- W1978732406 title "A strong - correlation in radio pulsars with implications for torque variations" @default.
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- W1978732406 doi "https://doi.org/10.1111/j.1745-3933.2006.00192.x" @default.
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