1E 2259+586
Comment: WP:NASTRO states, Template:Tq is only for quoting in talk and project pages. Do not use it in actual articles. and Template:Tq is only for quoting in talk and project pages. Do not use it in actual articles.. Also, the sources does not support much of the information, particularly the distance from Cassipeia and the anti-glitch claims. 🌀Hurricane Wind and Fire, why did you decline my draft? (talk) (contribs)🔥 21:41, 14 July 2026 (UTC)
1E 2259+586 is a type of neutron star that has a strong magnetic field called a magnetar.
This magnetar has a slowing rotation, which is called an “ Anti-Glitch “ because typically, neutron stars have increasing rotation rather than decreasing and the usual increase is called a “ Glitch “ ; hence the name.
10,000 light years away from the sun in the constellation Cassiopeia, 1E 2259+586 was discovered in 1981 by using X-Ray and Gamma Ray detection.
Not only does its magnetic field but also its topology affects the magnetar’s activity.[1]
References
- ↑ D. Pizzocaro; A. Tiengo; S. Mereghetti; R. Turolla; P. Esposito; L. Stella; S. Zane; N. Rea; F. Coti Zelati; G. Israel (7 June 2019). "Detailed X-ray spectroscopy of the magnetar 1E 2259+586" (PDF). doi:10.1051/0004-6361/201834784.
Book : The Universe ( By Lonely Planet )
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