Pulsar Glitches
Pulsar Glitches is an observed phenomenon in pulsar timing characterized by a sudden increase in rotational frequency followed by a gradual relaxation, distinguishing it from steady spin-down trends and other timing anomalies through its transient and unpredictable nature.
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2017–2026
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289
A study of 315 glitches in the rotation of 102 pulsars
C. M. Espinoza, A. G. Lyne, B. W. Stappers et al. · Monthly Notices of the Royal Astronomical Society · 2011 · 519 citations · Full text
Natural Sciences, Astronomy, Physics +11
B. Haskell, A. Melatos · International Journal of Modern Physics D · 2015 · 321 citations · Full text
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Commonwealth Scientific and Industrial Research Organisation, Australia
20 publications · 1.5K citations
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University of Manchester
Manchester, United Kingdom
35 h-index
130 publications
13.2K citations

Commonwealth Scientific and Industrial Research Organisation
Canberra, Australia
24 h-index
101 publications
7K citations
Australia Telescope National Facility
Sydney, Australia
24 h-index
96 publications
7K citations

McGill University
Montreal, Canada
22 h-index
45 publications
3.2K citations
Goddard Space Flight Center
Greenbelt, United States
21 h-index
43 publications
2.4K citations

The University of Melbourne
Melbourne, Australia
21 h-index
79 publications
4.2K citations
University of Southampton
Southampton, United Kingdom
20 h-index
32 publications
2.4K citations
Nicolaus Copernicus Astronomical Center
Warsaw, Poland
18 h-index
45 publications
1.7K citations
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ApJ · 73 publications · 5.9K citations
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95 publications · 6K citations
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PRL · 10 publications · 1.1K citations
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9 publications · 342 citations
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