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Article ; Online: Polarized x-rays from a magnetar.

Taverna, Roberto / Turolla, Roberto / Muleri, Fabio / Heyl, Jeremy / Zane, Silvia / Baldini, Luca / González-Caniulef, Denis / Bachetti, Matteo / Rankin, John / Caiazzo, Ilaria / Di Lalla, Niccolò / Doroshenko, Victor / Errando, Manel / Gau, Ephraim / Kırmızıbayrak, Demet / Krawczynski, Henric / Negro, Michela / Ng, Mason / Omodei, Nicola /
Possenti, Andrea / Tamagawa, Toru / Uchiyama, Keisuke / Weisskopf, Martin C / Agudo, Ivan / Antonelli, Lucio A / Baumgartner, Wayne H / Bellazzini, Ronaldo / Bianchi, Stefano / Bongiorno, Stephen D / Bonino, Raffaella / Brez, Alessandro / Bucciantini, Niccolò / Capitanio, Fiamma / Castellano, Simone / Cavazzuti, Elisabetta / Ciprini, Stefano / Costa, Enrico / De Rosa, Alessandra / Del Monte, Ettore / Di Gesu, Laura / Di Marco, Alessandro / Donnarumma, Immacolata / Dovčiak, Michal / Ehlert, Steven R / Enoto, Teruaki / Evangelista, Yuri / Fabiani, Sergio / Ferrazzoli, Riccardo / Garcia, Javier A / Gunji, Shuichi / Hayashida, Kiyoshi / Iwakiri, Wataru / Jorstad, Svetlana G / Karas, Vladimir / Kitaguchi, Takao / Kolodziejczak, Jeffery J / La Monaca, Fabio / Latronico, Luca / Liodakis, Ioannis / Maldera, Simone / Manfreda, Alberto / Marin, Frédéric / Marinucci, Andrea / Marscher, Alan P / Marshall, Herman L / Matt, Giorgio / Mitsuishi, Ikuyuki / Mizuno, Tsunefumi / Ng, Stephen C-Y / O'Dell, Stephen L / Oppedisano, Chiara / Papitto, Alessandro / Pavlov, George G / Peirson, Abel L / Perri, Matteo / Pesce-Rollins, Melissa / Pilia, Maura / Poutanen, Juri / Puccetti, Simonetta / Ramsey, Brian D / Ratheesh, Ajay / Romani, Roger W / Sgrò, Carmelo / Slane, Patrick / Soffitta, Paolo / Spandre, Gloria / Tavecchio, Fabrizio / Tawara, Yuzuru / Tennant, Allyn F / Thomas, Nicholas E / Tombesi, Francesco / Trois, Alessio / Tsygankov, Sergey S / Vink, Jacco / Wu, Kinwah / Xie, Fei

Science (New York, N.Y.)

2022  Volume 378, Issue 6620, Page(s) 646–650

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 ... ...

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 ~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.
Language English
Publishing date 2022-11-03
Publishing country United States
Document type Journal Article ; Research Support, Non-U.S. Gov't ; Research Support, U.S. Gov't, Non-P.H.S.
ZDB-ID 128410-1
ISSN 1095-9203 ; 0036-8075
ISSN (online) 1095-9203
ISSN 0036-8075
DOI 10.1126/science.add0080
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