학술논문

Discovery of a variable energy-dependent X-ray polarization in the accreting neutron star GX 5-1
Document Type
Working Paper
Author
Fabiani, SergioCapitanio, FiammaIaria, RosarioPoutanen, JuriGnarini, AndreaUrsini, FrancescoFarinelli, RubenBobrikova, AnnaSteiner, James F.Svoboda, JiriAnitra, AlessioBaglio, Maria C.Carotenuto, FrancescoDel Santo, MelaniaFerrigno, CarloLewis, FraserRussell, David M.Russell, Thomas D.Eijnden, Jakob van denCocchi, MassimoDi Marco, AlessandroLa Monaca, FabioLiu, KuanRankin, JohnWeisskopf, Martin C.Xie, FeiBianchi, StefanoBurderi, LucianoDi Salvo, TizianaEgron, EliseIlliano, GiuliaKaaret, PhilipMatt, GiorgioMikušincová, RomanaMuleri, FabioPapitto, AlessandroAgudo, IvánAntonelli, Lucio A.Bachetti, MatteoBaldini, LucaBaumgartner, Wayne H.Bellazzini, RonaldoBongiorno, Stephen D.Bonino, RaffaellaBrez, AlessandroBucciantini, NiccolòCastellano, SimoneCavazzuti, ElisabettaChen, Chien-TingCiprini, StefanoCosta, EnricoDe Rosa, AlessandraDel Monte, EttoreDi Gesu, LauraDi Lalla, NiccolòDonnarumma, ImmacolataDoroshenko, VictorDovčiak, MichalEhlert, Steven R.Enoto, TeruakiEvangelista, YuriFerrazzoli, RiccardoGarcia, Javier A.Gunji, ShuichiHayashida, KiyoshiHeyl, JeremyIwakiri, WataruJorstad, Svetlana G.Karas, VladimirKislat, FabianKitaguchi, TakaoKolodziejczak, Jeffery J.Krawczynski, HenricLatronico, LucaLiodakis, IoannisMaldera, SimoneManfreda, AlbertoMarin, FrédéricMarinucci, AndreaMarscher, Alan P.Marshall, Herman L.Massaro, FrancescoMitsuishi, IkuyukiMizuno, TsunefumiNegro, MichelaNg, Chi-YungO'Dell, Stephen L.Omodei, NicolaOppedisano, ChiaraPavlov, George G.Peirson, Abel L.Perri, MatteoPesce-Rollins, MelissaPetrucci, Pierre-OlivierPilia, MauraPossenti, AndreaPuccetti, SimonettaRamsey, Brian D.Ratheesh, AjayRoberts, Oliver J.Romani, Roger W.Sgrò, CarmeloSlane, PatrickSoffitta, PaoloSpandre, GloriaSwartz, Douglas A.Tamagawa, ToruTavecchio, FabrizioTaverna, RobertoTawara, YuzuruTennant, Allyn F.Thomas, Nicholas E.Tombesi, FrancescoTrois, AlessioTsygankov, Sergey S.Turolla, RobertoVink, JaccoWu, KinwahZane, Silvia
Source
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
Abstract
We report on the coordinated observations of the neutron star low-mass X-ray binary (NS-LMXB) \gx in X-rays (IXPE, NICER, Nustar and INTEGRAL), optical (REM and LCO), near-infrared (REM), mid-infrared (VLT VISIR), and radio (ATCA). This Z-source was observed by \IXPE twice in March-April 2023 (Obs. 1 and 2). In the radio band, the source was detected, but only upper-limits to the linear polarization were obtained at a $3\sigma$ level of $6.1\%$ at 5.5 GHz and $5.9\%$ at 9 GHz in Obs.~1 and $12.5\%$ at 5.5~GHz and $20\%$ at 9~GHz in Obs.~2. The mid-IR, near-IR and optical observations suggest the presence of a compact jet which peaks in the mid- or far-IR. The X-ray polarization degree was found to be $3.7\% \pm 0.4 \%$ (at $90\%$ confidence level) during Obs.~1 when the source was in the horizontal branch of the Z-track and $1.8\% \pm 0.4 \%$ during Obs.~2 when the source was in the normal-flaring branch. These results confirm the variation of polarization degree as a function of the position of the source in the color-color diagram as for previously observed Z-track sources (Cyg~X-2 and XTE~1701$-$462). Evidence for a variation of the polarization angle $\sim 20^\circ$ with energy is found in both observations, likely related to the different, non-orthogonal polarization angles of the disk and Comptonization components which peak at different energies.
Comment: Submitted to Astronomy and Astrophysics on 06 July 2023. Accepted on 21 November 2023