Observations of the magnetars 4U 0142+61 and 1E 2259+586 with the MAGIC telescopes
Context. Magnetars are an extreme, highly magnetized class of isolated neutron stars whose large X-ray luminosity is believed to be driven by their high magnetic field. Aims: We study for the first time the possible very high energy γ-ray emission above 100 GeV from magnetars, observing the sources 4U 0142+61 and 1E 2259+586. Methods: We observed
Backes, M. et al.
Fecha de publicación:
1
2013