Physics
Scientific paper
Apr 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987natur.326..569l&link_type=abstract
Nature (ISSN 0028-0836), vol. 326, April 9, 1987, p. 569-571.
Physics
66
Angular Velocity, Pulsars, Stellar Evolution, Stellar Rotation, Neutron Stars, Stellar Spectrophotometry
Scientific paper
Many pulsars display irregularities in rotation rate of two main types: random fluctuations, known as timing noise, and discrete discontinuities in rotation rate, known as glitches. The author discribes a recent series of observations in which the relatively old pulsar PSR 0355+54 has been seen to suffer two glitches, the second of which is the largest observed in any pulsar and provides a valuable opportunity for the study of the recovery of the interior of a neutron star following such a large perturbation.
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