Title an Anti-Glitch in a Magnetar Author(S) Archibald, RF
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by HKU Scholars Hub Title An anti-glitch in a magnetar Archibald, R. F.; Kaspi, V. M.; Ng, SCY; Gourgouliatos, K. N.; Author(s) Tsang, D.; Scholz, P.; Beardmore, A. P.; Gehrels, N.; Kennea, J. A. Citation Nature, 2013, v. 497 n. 7451, p. 591-593 Issued Date 2013 URL http://hdl.handle.net/10722/186148 Rights Creative Commons: Attribution 3.0 Hong Kong License An Anti-Glitch in a Magnetar R. F. Archibald1, V. M. Kaspi1, C. -Y. Ng1,2, K. N. Gourgouliatos 1, D. Tsang1, P. Scholz1, A. P. Beardmore3, N. Gehrels4, & J. A. Kennea5 1Department of Physics, McGill University, Montreal QC, H3A 2T8, Canada 2Department of Physics, The University of Hong Kong, Pokfulam Road, Hong Kong 3Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK 4Astrophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771 USA 5Department of Astronomy and Astrophysics, 525 Davey Lab, Pennsylvania State University, Uni- versity Park, PA 16802, USA Magnetars are neutron stars showing dramatic X-ray and soft γ-ray outbursting behaviour that is thought to be powered by intense internal magnetic fields1. Like conventional young neutron stars in the form of radio pulsars, magnetars exhibit “glitches” during which angu- lar momentum is believed to be transferred between the solid outer crust and the superfluid component of the inner crust 2–4. Hitherto, the several hundred observed glitches in ra- dio pulsars5, 6 and magnetars7 have involved a sudden spin-up of the star, due presumably to the interior superfluid rotating faster than the crust.
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