Three charts from the world of research, selected by Nature editors.
the magnetic field left behind by a dead star
. In the remnant of a supernova, the core of the dead star emits a particle wind that gyrates within a magnetic field that is typically doughnut-shaped, and accelerates the particles to ultra-high energies, generating a gas cloud called a pulsar wind nebula. The onset of the wind is known as the termination shock; the reverse shock acts in the opposite direction as the nebula ages.
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