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- W2081018854 startingPage "473" @default.
- W2081018854 abstract "We present the results of 6.5 years of timing observations of PSR 0655 + 64 and derive an ephemeris and precise position. The very small period derivative of |$6.9 times {10}^{-19},text{s},{text{s}}^{-1}$| implies a spin-down age of |$4.5 times {10}^{9},text{yr}$| and a magnetic field of |$1.2 times {10}^{10},text{G}$|. Kulkarni's optical identification of the companion star is confirmed. The measured eccentricity of |$7.5 times {10}^{-6}$| may be partly due to a general relativistic delay caused by the passage of pulses through the gravitational field of the companion star. A significant relativistic advance of the periastron should be observable over a period of ≲ 30 yr." @default.
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- W2081018854 date "1988-06-01" @default.
- W2081018854 modified "2023-09-23" @default.
- W2081018854 title "Timing observations of the binary pulsar PSR 0655 + 64" @default.
- W2081018854 doi "https://doi.org/10.1093/mnras/232.3.473" @default.
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