2006/07/12 by T. V. Shabanova, Tatiana V. Shabanova · 1 citation
Earth and Planetary Sciences · Physics and Astronomy · #Geophysics and Gravity Measurements #High-pressure geophysics and materials #Pulsars and Gravitational Waves Research #astro-ph
paper · pdf · doi:10.1007/s10509-007-9302-5
published as Astrophys.SpaceSci.308:591-593,2007 · 3 pages, 2 figures. Accepted by Astrophysics and Space Science. Contribution to the proceedings of Isolated Neutron Stars, London, 2006
arxiv created 2006/07/12 · openalex publication_date 2007/03/20 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/29
The pulsar B1822-09 (J1825-0935) experienced a series of five unusual slow glitches over the 1995-2004 interval. The results of further study of this unusual glitch phenomenon are presented. It is also reported the detection a new glitch of typical signature that occurred in the pulsar period in 2006 January.