Properties and observability of glitches and anti-glitches in accreting pulsars
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201525667/pdf
Reference39 articles.
1. Narrow-band search of continuous gravitational-wave signals from Crab and Vela pulsars in Virgo VSR4 data
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4. INTEGRAL observations of the variability of OAO 1657-415
5. Neutron starquakes and pulsar speedup
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1. Discovery of the First Antiglitch Event in the Rotation-powered Pulsar PSR B0540-69;The Astrophysical Journal Letters;2024-05-01
2. Gapless Neutron Superfluidity Can Explain the Late Time Cooling of Transiently Accreting Neutron Stars;Physical Review Letters;2024-04-29
3. Accreting Strongly Magnetized Neutron Stars: X-ray Pulsars;Handbook of X-ray and Gamma-ray Astrophysics;2024
4. Continuous gravitational waves from trapped magnetar ejecta and the connection to glitches and antiglitches;Monthly Notices of the Royal Astronomical Society;2023-11-02
5. Accreting Strongly Magnetized Neutron Stars: X-ray Pulsars;Handbook of X-ray and Gamma-ray Astrophysics;2023
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