학술논문

Discovery of X-ray Polarization from the Black Hole Transient Swift J1727.8-1613
Document Type
Working Paper
Author
Veledina, AlexandraMuleri, FabioDovciak, MichalPoutanen, JuriRatheesh, AjayCapitanio, FiammaMatt, GiorgioSoffitta, PaoloTennant, Allyn F.Negro, MichelaKaaret, PhilipCosta, EnricoIngram, AdamSvoboda, JiriKrawczynski, HenricBianchi, StefanoSteiner, James F.Garcia, Javier A.Kravtsov, VadimNitindala, Anagha P.Ewing, MelissaMastroserio, GuglielmoMarinucci, AndreaUrsini, FrancescoTombesi, FrancescoTsygankov, Sergey S.Yang, Yi-JungWeisskopf, Martin C.Trushkin, Sergei A.Egron, EliseIacolina, Maria NoemiPilia, MauraMarra, LorenzoMikusincova, RomanaNathan, EdwardParra, MaximePetrucci, Pierre-OlivierPodgorny, JakubTugliani, StefanoZane, SilviaZhang, WendaAgudo, IvanAntonelli, Lucio A.Bachetti, MatteoBaldini, LucaBaumgartner, Wayne H.Bellazzini, RonaldoBongiorno, Stephen D.Bonino, RaffaellaBrez, AlessandroBucciantini, NiccoloCastellano, SimoneCavazzuti, ElisabettaChen, Chien-TingCiprini, StefanoDe Rosa, AlessandraDel Monte, EttoreDi Gesu, LauraDi Lalla, NiccoloDi Marco, AlessandroDonnarumma, ImmacolataDoroshenko, VictorEhlert, Steven R.Enoto, TeruakiEvangelista, YuriFabiani, SergioFerrazzoli, RiccardoGunji, ShuichiHayashida, KiyoshiHeyl, JeremyIwakiri, WataruJorstad, Svetlana G.Karas, VladimirKislat, FabianKitaguchi, TakaoKolodziejczak, Jeffery J.La Monaca, FabioLatronico, LucaLiodakis, IoannisMaldera, SimoneManfreda, AlbertoMarin, FredericMarscher, Alan P.Marshall, Herman L.Massaro, FrancescoMitsuishi, IkuyukiMizuno, TsunefumiNg, Chi-YungO'Dell, Stephen L.Omodei, NicolaOppedisano, ChiaraPapitto, AlessandroPavlov, George G.Peirson, Abel L.Perri, MatteoPesce-Rollins, MelissaPossenti, AndreaPuccetti, SimonettaRamsey, Brian D.Rankin, JohnRoberts, Oliver J.Romani, Roger W.Sgro, CarmeloSlane, PatrickSpandre, GloriaSwartz, Douglas A.Tamagawa, ToruTavecchio, FabrizioTaverna, RobertoTawara, YuzuruThomas, Nicholas E.Trois, AlessioTurolla, RobertoVink, JaccoWu, KinwahXie, Fei
Source
Subject
Astrophysics - High Energy Astrophysical Phenomena
Astrophysics - Solar and Stellar Astrophysics
Language
Abstract
We report the first detection of the X-ray polarization of the bright transient Swift J1727.8-1613 with the Imaging X-ray Polarimetry Explorer. The observation was performed at the beginning of the 2023 discovery outburst, when the source resided in the bright hard state. We find a time- and energy-averaged polarization degree of 4.1%+/-0.2% and a polarization angle of 2.2+/-1.3 degrees (errors at 68% confidence level; this translates to about 20-sigma significance of the polarization detection). This finding suggests that the hot corona emitting the bulk of the detected X-rays is elongated, rather than spherical. The X-ray polarization angle is consistent with that found in sub-mm wavelengths. Since the sub-mm polarization was found to be aligned with the jet direction in other X-ray binaries, this indicates that the corona is elongated orthogonal to the jet.
Comment: 10 pages, 3 figures, submitted