Magnetars are a kind of neutron star which can be characterised by their extremely robust magnetic fields. These fields are estimated to be a thousand billion instances stronger than the magnetic area of the Earth, making magnetars a number of the most magnetic objects within the universe. They emit intense bursts of X-rays and gamma rays, which might final from a fraction of a second to a number of minutes, and are regarded as brought on by the discharge of power saved of their magnetic fields. In addition, magnetars additionally emit a steady low-level emission of X-rays.
A current publication within the journal Nature Astronomy is providing new insights into magnetars, whose traits are nonetheless not properly understood. A magnetar is a kind of neutron star with a magnetic field that is extremely strong and rotates once every two to ten seconds.
Researchers observing the magnetar SGR 1935+2154 detected a sudden slowing of the star’s angular momentum, often referred to as a spin-down glitch, on October 5, 2020. In the following days, the magnetar emitted three Fast Radio Burst-like radio bursts followed by a month-long episode of pulsed radio emission, despite there being no signs of variation in the X-ray emission behavior in the star or evidence of a strong X-ray burst.
Due to the rarity of spin-down glitches and radio signals from magnetars, the research team says the synchronicity of these events suggests an association, offering clues to their origin and triggering mechanisms.
The researchers point to plasma shedding close to the magnetic pole, which generated a wind that impacted the star’s momentum and magnetic field and created the combination needed to trigger radio emission.
Reference: “Magnetar spin-down glitch clearing the way for FRB-like bursts and a pulsed radio episode” by G. Younes, M. G. Baring, A. K. Harding, T. Enoto, Z. Wadiasingh, A. B. Pearlman, W. C. G. Ho, S. Guillot, Z. Arzoumanian, A. Borghese, K. Gendreau, E. Göğüş, T. Güver, A. J. van der Horst, C.-P. Hu, G. K. Jaisawal, C. Kouveliotou, L. Lin and W. A. Majid, 12 January 2023, Nature Astronomy.
DOI: 10.1038/s41550-022-01865-y
