Magnetar spin-down
WebWe find that if magnetars are born rapidly rotating, with initial spin periods (P) of ~1 ms, then of order 10 51 -10 52 ergs of rotational energy can be extracted in ~10 s. If magnetars … Web(MAGNESIA: Magnetar census: the impact of highly magnetic neutron stars in the explosive and transient Universe). The aim of my PhD project is to search for pulsars and …
Magnetar spin-down
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WebDuring magnetar outburst, a decaying flux, shrink hotspot, decaying torque, spin-down glitch, softening spectra, etc. are often seen (Kaspi & Beloborodov 2024; Coti Zelati et al. … Web1 apr. 2011 · We explore fallback accretion onto newly born magnetars during the supernova of massive stars. Strong magnetic fields (∼1015 G) and short spin periods …
Web9 aug. 2024 · A newly born magnetar is thought to be central engine of some long gamma-ray bursts (GRBs). We investigate the evolution of the electromagnetic (EM) emission … Web25 mrt. 2024 · The magnetar SGR 1935+2154 is reported to have an antiglitch (i.e.,spin-down event) (Younes et al.2024).The antiglitch is also followed by fast radio bursts and pulsed radio emission (Younes et al.2024;Good &CHIME/FRB Collaboration 2024;Zhu et al.2024).This will make SGR 1935+2154 the sixth magnetar to show pulsed radio …
WebMagnetar Spin-Down demosthenes kazanas 1999, Astrophysical Journal We examine the effects of a relativistic wind on the spin down of a neutron star and apply our results to … Web13 feb. 2024 · A magnetar is a type of neutron star with a magnetic field that is extremely strong and rotates once every two to ten seconds. Researchers observing the magnetar …
Web29 mei 2013 · Here we report X-ray timing observations of the magnetar 1E 2259+586 (ref. 8 ), which exhibited a clear ‘anti-glitch’—a sudden spin-down. We show that this event, …
WebA magnetar is a type of neutron star with an extremely powerful magnetic field (∼10 9 to 10 11 T, ∼10 13 to 10 15 G). The magnetic-field decay powers the emission of high-energy … 68折扣WebSuch energetic particle winds will also a ect the spin-down torque of the star by distorting the dipole eld structure near the light cylinder (Thompson & Blaes 1998 [TB98]). We will … 68才 仕事Web6 apr. 2024 · Among magnetar models of fast radio bursts (FRBs), there is ongoing debate about whether the site of coherent radio emission lies within or beyond the light cylinder. We propose a 68拍是什么意思啊Web12 jan. 2024 · Many attributes of magnetars remain poorly understood: spin-down glitches or the sudden reductions in the star’s angular momentum, radio bursts reminiscent of … 68按键测试Web1 sep. 2015 · If the spin-down power is injected into the forward shock, then we expect an “external” plateau. Dall'Osso et al. (2011) proposed an analytic treatment to account for … 68拍怎么打拍子Web16 sep. 2024 · Worked with Dr. Griffin Hosseinzadeh under the supervision of Prof. Edo Berger to model a sample of hydrogen-poor superluminous supernovae (SLSNe) from … 68文献馆WebCan magnetar spin-down power extended emission in some short GRBs? Journal Monthly Notices of the Royal Astronomical Society Volume Issue number 431 2 Pages (from … 68拍 節拍器