Optical pulse timing observations of the young pulsar PSR 0540-69 in the LMC using the 4-m Anglo-Australian Telescope over a 2-yr intervalhave yielded accurate period parameters for the pulsar. The derivedvalue of the braking index is 2.01 + or - 0.02, much less than themagnetic-dipole value of 3.0.
CITATION STYLE
Manchester, R. N., & Peterson, B. A. (1989). A braking index for PSR 0540-69. The Astrophysical Journal, 342, L23. https://doi.org/10.1086/185475
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