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Polarized x-rays from a magnetar.

Roberto TavernaRoberto TurollaFabio MuleriJeremy HeylSilvia ZaneLuca BaldiniDenis González-CaniulefMatteo BachettiJohn RankinIlaria CaiazzoNiccoló Di LallaVictor DoroshenkoManel ErrandoEphraim GauDemet KırmızıbayrakHenric KrawczynskiMichela NegroMason NgNicola OmodeiAndrea PossentiToru TamagawaKeisuke UchiyamaMartin C WeisskopfIvan AgudoLucio A AntonelliWayne H BaumgartnerRonaldo BellazziniStefano BianchiStephen D BongiornoRaffaella BoninoAlessandro BrezNiccolò BucciantiniFiamma CapitanioSimone CastellanoElisabetta CavazzutiStefano CipriniEnrico CostaAlessandra De RosaEttore Del MonteLaura Di GesuAlessandro Di MarcoImmacolata DonnarummaMichal DovčiakSteven R EhlertTeruaki EnotoYuri EvangelistaSergio FabianiRiccardo FerrazzoliJavier A GarciaShuichi GunjiKiyoshi HayashidaWataru IwakiriSvetlana G JorstadVladimir KarasTakao KitaguchiJeffery J KolodziejczakFabio La MonacaLuca LatronicoIoannis LiodakisSimone MalderaAlberto ManfredaFrédéric MarinAndrea MarinucciAlan P MarscherHerman L MarshallGiorgio MattIkuyuki MitsuishiTsunefumi MizunoStephen C-Y NgStephen L O'DellChiara OppedisanoAlessandro PapittoGeorge G PavlovAbel L PeirsonMatteo PerriMelissa Pesce-RollinsMaura PiliaJuri PoutanenSimonetta PuccettiBrian D RamseyAjay RatheeshRoger W RomaniCarmelo SgróPatrick SlanePaolo SoffittaGloria SpandreFabrizio TavecchioYuzuru TawaraAllyn F TennantNicholas E ThomasFrancesco TombesiAlessio TroisSergey S TsygankovJacco VinkKinwah WuFei Xie
Published in: Science (New York, N.Y.) (2022)
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 ~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° at ~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.
Keyphrases
  • high resolution
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  • contrast enhanced