The detection of polarized X-ray emission from the magnetar 1E 2259+586
Heyl Jeremy; Taverna Roberto; Turolla Roberto; Israel Gian Luca; Ng Mason; Kırmızıbayrak Demet; González-Caniulef Denis; Caiazzo Ilaria; Zane Silvia; Ehlert Steven R; Negro Michela; Agudo Iván; Antonelli Lucio Angelo; Bachetti Matteo; Baldini Luca; Baumgartner Wayne H; Bellazzini Ronaldo; Bianchi Stefano; Bongiorno Stephen D; Bonino Raffaella; Brez Alessandro; Bucciantini Niccolò; Capitanio Fiamma; Castellano Simone; Cavazzuti Elisabetta; Chen Chien-Ting; Ciprini Stefano; Costa Enrico; De Rosa Alessandra; Del Monte Ettore; Di Gesu Laura; Di Lalla Niccolò; Di Marco Alessandro; Donnarumma Immacolata; Doroshenko Victor; Dovčiak Michal; Enoto Teruaki; Evangelista Yuri; Fabiani Sergio; Ferrazzoli Riccardo; Garcia Javier A; Gunji Shuichi; Hayashida Kiyoshi; Iwakiri Wataru; Jorstad Svetlana G; Kaaret Philip; Karas Vladimir; Kislat Fabian; Kitaguchi Takao; Kolodziejczak Jeffery J; Krawczynski Henric; Monaca Fabio La; Latronico Luca; Liodakis Ioannis; Maldera Simone; Manfreda Alberto; Marin Frédéric; Marinucci Andrea; Marscher Alan P; Marshall Herman L; Massaro Francesco; Matt Giorgio; Mitsuishi Ikuyuki; Mizuno Tsunefumi; Muleri Fabio; Ng C-Y; O’Dell Stephen L; Omodei Nicola; Oppedisano Chiara; Papitto Alessandro; Pavlov George G; Peirson Abel Lawrence; Perri Matteo; Pesce-Rollins Melissa; Petrucci Pierre-Olivier; Pilia Maura; Possenti Andrea; Poutanen Juri; Puccetti Simonetta; Ramsey Brian D; Rankin John; Ratheesh Ajay; Roberts Oliver J; Romani Roger W; Sgrò Carmelo; Slane Patrick; Soffitta Paolo; Spandre Gloria; Swartz Douglas A; Tamagawa Toru; Tavecchio Fabrizio; Tawara Yuzuru; Tennant Allyn F; Thomas Nicholas E; Tombesi Francesco; Trois Alessio; Tsygankov Sergey S; Vink Jacco; Weisskopf Martin C; Wu Kinwah; Xie Fei
The detection of polarized X-ray emission from the magnetar 1E 2259+586
Oxford University Press
Julkaisun pysyvä osoite on:
https://urn.fi/URN:NBN:fi-fe2025082789341
https://urn.fi/URN:NBN:fi-fe2025082789341
Tiivistelmä
We report on IXPE, NICER, and XMM–Newton observations of the magnetar 1E 2259+586. We find that the source is significantly polarized at about or above 20 per cent for all phases except for the secondary peak where it is more weakly polarized. The polarization degree is strongest during the primary minimum which is also the phase where an absorption feature has been identified previously. The polarization angle of the photons are consistent with a rotating vector model with a mode switch between the primary minimum and the rest of the rotation of the neutron star. We propose a scenario in which the emission at the source is weakly polarized (as in a condensed surface) and, as the radiation passes through a plasma arch, resonant cyclotron scattering off of protons produces the observed polarized radiation. This confirms the magnetar nature of the source with a surface field greater than about 1015 G.
Kokoelmat
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