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Decrease in the Period of Pulsar PSR 0833–45

Abstract

A DECREASE of 196 ns in the period of pulsar PSR 0833–45 has recently been observed1,2; I suggest that this decrease results from the addition of mass to the pulsar. A remnant of the supernova explosion forming the pulsar may not have escaped the gravitational field and may now have fallen back on the pulsar.

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References

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DURNEY, B. Decrease in the Period of Pulsar PSR 0833–45. Nature 222, 1260–1261 (1969). https://doi.org/10.1038/2221260a0

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