Polarized x-rays from a magnetar

Taverna, Roberto; Turolla, Roberto; Muleri, Fabio; Heyl, Jeremy; Zane, Silvia; Baldini, Luca; Gonzalez-Caniulef, Denis; Bachetti, Matteo; Rankin, John; Caiazzo, Ilaria; Di Lalla, Niccolo; Doroshenko, Victor; Errando, Manel; Gau, Ephraim; Kirmizibayrak, Demet; et. al.

Abstract

Magnetars are neutron stars with ultrastrong magnetic fields, which can be observed in x-rays. Polarization measurements could provide information on their magnetic fields and surface properties. We observed polarized x-rays from the magnetar 4U 0142+61 using the Imaging X-ray Polarimetry Explorer and found a linear polarization degree of 13.5 +/- 0.8% averaged over the 2- to 8-kilo-electron volt band. The polarization changes with energy: The degree is 15.0 +/- 1.0% at 2 to 4 kilo-electron volts, drops below the instrumental sensitivity similar to 4 to 5 kilo-electron volts, and rises to 35.2 +/- 7.1% at 5.5 to 8 kilo-electron volts. The polarization angle also changes by 90 degrees at similar to 4 to 5 kilo-electron volts. These results are consistent with a model in which thermal radiation from the magnetar surface is reprocessed by scattering off charged particles in the magnetosphere.

Más información

Título según WOS: ID WOS:000898883700012 Not found in local WOS DB
Título de la Revista: SCIENCE
Volumen: 378
Número: 6620
Editorial: AMER ASSOC ADVANCEMENT SCIENCE
Fecha de publicación: 2022
Página de inicio: 646
Página final: 649
DOI:

10.1126/science.add0080

Notas: ISI