eprintid: 10186701
rev_number: 7
eprint_status: archive
userid: 699
dir: disk0/10/18/67/01
datestamp: 2024-02-07 11:48:00
lastmod: 2024-02-07 11:48:00
status_changed: 2024-02-07 11:48:00
type: article
metadata_visibility: show
sword_depositor: 699
creators_name: Heyl, J
creators_name: Taverna, R
creators_name: Turolla, R
creators_name: Israel, GL
creators_name: Ng, M
creators_name: Kırmızıbayrak, D
creators_name: González-Caniulef, D
creators_name: Caiazzo, I
creators_name: Zane, S
creators_name: Ehlert, SR
creators_name: Negro, M
creators_name: Agudo, I
creators_name: Antonelli, LA
creators_name: Bachetti, M
creators_name: Baldini, L
creators_name: Baumgartner, WH
creators_name: Bellazzini, R
creators_name: Bianchi, S
creators_name: Bongiorno, SD
creators_name: Bonino, R
creators_name: Brez, A
creators_name: Bucciantini, N
creators_name: Capitanio, F
creators_name: Castellano, S
creators_name: Cavazzuti, E
creators_name: Chen, CT
creators_name: Ciprini, S
creators_name: Costa, E
creators_name: De Rosa, A
creators_name: Monte, ED
creators_name: Gesu, LD
creators_name: Lalla, ND
creators_name: Marco, AD
creators_name: Donnarumma, I
creators_name: Doroshenko, V
creators_name: Dovčiak, M
creators_name: Enoto, T
creators_name: Evangelista, Y
creators_name: Fabiani, S
creators_name: Ferrazzoli, R
creators_name: Garcia, JA
creators_name: Gunji, S
creators_name: Hayashida, K
creators_name: Iwakiri, W
creators_name: Jorstad, SG
creators_name: Kaaret, P
creators_name: Karas, V
creators_name: Kislat, F
creators_name: Kitaguchi, T
creators_name: Kolodziejczak, JJ
creators_name: Krawczynski, H
creators_name: Monaca, FL
creators_name: Latronico, L
creators_name: Liodakis, I
creators_name: Maldera, S
creators_name: Manfreda, A
creators_name: Marin, F
creators_name: Marinucci, A
creators_name: Marscher, AP
creators_name: Marshall, HL
creators_name: Massaro, F
creators_name: Matt, G
creators_name: Mitsuishi, I
creators_name: Mizuno, T
creators_name: Muleri, F
creators_name: Ng, CY
creators_name: O’Dell, SL
creators_name: Omodei, N
creators_name: Oppedisano, C
creators_name: Papitto, A
creators_name: Pavlov, GG
creators_name: Peirson, AL
creators_name: Perri, M
creators_name: Pesce-Rollins, M
creators_name: Petrucci, PO
creators_name: Pilia, M
creators_name: Possenti, A
creators_name: Poutanen, J
creators_name: Puccetti, S
creators_name: Ramsey, BD
creators_name: Rankin, J
creators_name: Ratheesh, A
creators_name: Roberts, OJ
creators_name: Romani, RW
creators_name: Sgrò, C
creators_name: Slane, P
creators_name: Soffitta, P
creators_name: Spandre, G
creators_name: Swartz, DA
creators_name: Tamagawa, T
creators_name: Tavecchio, F
creators_name: Tawara, Y
creators_name: Tennant, AF
creators_name: Thomas, NE
creators_name: Tombesi, F
creators_name: Trois, A
creators_name: Tsygankov, SS
creators_name: Vink, J
creators_name: Weisskopf, MC
creators_name: Wu, K
title: The detection of polarized X-ray emission from the magnetar 1E 2259+586
ispublished: pub
divisions: UCL
divisions: B04
divisions: C06
divisions: F63
keywords: polarization, techniques: polarimetric, stars: magnetars, pulsars: individual: 1E 2259+586
note: © The Author(s) 2023.
Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative
Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium,
provided the original work is properly cited.
abstract: 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.
date: 2024-02-01
date_type: published
publisher: Oxford University Press (OUP)
official_url: http://dx.doi.org/10.1093/mnras/stad3680
oa_status: green
full_text_type: pub
language: eng
primo: open
primo_central: open_green
verified: verified_manual
elements_id: 2216455
doi: 10.1093/mnras/stad3680
lyricists_name: Zane, Silvia
lyricists_name: Wu, Kinwah
lyricists_id: SZANE58
lyricists_id: KWUXX50
actors_name: Kalinowski, Damian
actors_id: DKALI47
actors_role: owner
full_text_status: public
publication: Monthly Notices of the Royal Astronomical Society
volume: 527
number: 4
pagerange: 12219-12231
issn: 0035-8711
citation:        Heyl, J;    Taverna, R;    Turolla, R;    Israel, GL;    Ng, M;    Kırmızıbayrak, D;    González-Caniulef, D;                                                                                                                                                                                                                                                                                                                                                                                     ... Wu, K; + view all <#>        Heyl, J;  Taverna, R;  Turolla, R;  Israel, GL;  Ng, M;  Kırmızıbayrak, D;  González-Caniulef, D;  Caiazzo, I;  Zane, S;  Ehlert, SR;  Negro, M;  Agudo, I;  Antonelli, LA;  Bachetti, M;  Baldini, L;  Baumgartner, WH;  Bellazzini, R;  Bianchi, S;  Bongiorno, SD;  Bonino, R;  Brez, A;  Bucciantini, N;  Capitanio, F;  Castellano, S;  Cavazzuti, E;  Chen, CT;  Ciprini, S;  Costa, E;  De Rosa, A;  Monte, ED;  Gesu, LD;  Lalla, ND;  Marco, AD;  Donnarumma, I;  Doroshenko, V;  Dovčiak, M;  Enoto, T;  Evangelista, Y;  Fabiani, S;  Ferrazzoli, R;  Garcia, JA;  Gunji, S;  Hayashida, K;  Iwakiri, W;  Jorstad, SG;  Kaaret, P;  Karas, V;  Kislat, F;  Kitaguchi, T;  Kolodziejczak, JJ;  Krawczynski, H;  Monaca, FL;  Latronico, L;  Liodakis, I;  Maldera, S;  Manfreda, A;  Marin, F;  Marinucci, A;  Marscher, AP;  Marshall, HL;  Massaro, F;  Matt, G;  Mitsuishi, I;  Mizuno, T;  Muleri, F;  Ng, CY;  O’Dell, SL;  Omodei, N;  Oppedisano, C;  Papitto, A;  Pavlov, GG;  Peirson, AL;  Perri, M;  Pesce-Rollins, M;  Petrucci, PO;  Pilia, M;  Possenti, A;  Poutanen, J;  Puccetti, S;  Ramsey, BD;  Rankin, J;  Ratheesh, A;  Roberts, OJ;  Romani, RW;  Sgrò, C;  Slane, P;  Soffitta, P;  Spandre, G;  Swartz, DA;  Tamagawa, T;  Tavecchio, F;  Tawara, Y;  Tennant, AF;  Thomas, NE;  Tombesi, F;  Trois, A;  Tsygankov, SS;  Vink, J;  Weisskopf, MC;  Wu, K;   - view fewer <#>    (2024)    The detection of polarized X-ray emission from the magnetar 1E 2259+586.                   Monthly Notices of the Royal Astronomical Society , 527  (4)   pp. 12219-12231.    10.1093/mnras/stad3680 <https://doi.org/10.1093/mnras%2Fstad3680>.       Green open access   
 
document_url: https://discovery.ucl.ac.uk/id/eprint/10186701/1/Zane_The%20detection%20of%20polarized%20X-ray%20emission%20from%20the%20magnetar_VoR.pdf