학술논문

First X-ray polarization measurement confirms the low black-hole spin in LMC X-3
Document Type
Working Paper
Author
Svoboda, JiříDovčiak, MichalSteiner, James F.Muleri, FabioIngram, AdamYilmaz, AnastasiyaCavero, Nicole RodriguezMarra, LorenzoPoutanen, JuriVeledina, AlexandraMojaver, Mehrnoosh RahbardarBianchi, StefanoGarcia, JavierKaaret, PhilipKrawczynski, HenricMatt, GiorgioPodgorný, JakubWeisskopf, Martin C.Kislat, FabianPetrucci, Pierre-OlivierBrigitte, MaimounaBursa, MichalFabiani, SergioHu, KunChun, SoheeMastroserio, GuglielmoMikušincová, RomanaRatheesh, AjayRomani, Roger W.Soffitta, PaoloUrsini, FrancescoZane, SilviaAgudo, IvánAntonelli, Lucio A.Bachetti, MatteoBaldini, LucaBaumgartner, Wayne H.Bellazzini, RonaldoBongiorno, Stephen D.Bonino, RaffaellaBrez, AlessandroBucciantini, NiccoloCapitanio, FiammaCastellano, SimoneCavazzuti, ElisabettaChen, Chien-TingCiprini, StefanoCosta, EnricoDe Rosa, AlessandraDel Monte, EttoreDi Gesu, LauraDi Lalla, NiccoloDi Marco, AlessandroDonnarumma, ImmacolataDoroshenko, VictorEhlert, StevenEnoto, TeruakiEvangelista, YuriFerrazzoli, RiccardoGunji, ShuichiHayashida, KiyoshiHeyl, JeremyIwakiri, WataruJorstad, Svetlana G.Karas, VladimírKitaguchi, TakaoKolodziejczak, JefferyLa Monaca, FabioLatronico, LucaLiodakis, IoannisMaldera, SimoneManfreda, AlbertoMarin, FrédéricMarinucci, AndreaMarscher, Alan P.Marshall, Herman L.Massaro, FrancescoMitsuishi, IkuyukiMizuno, TsunefumiNegro, MichelaNg, C. -Y.O'Dell, Stephen L.Omodei, NicolaOppedisano, ChiaraPapitto, AlessandroPavlov, GeorgePeirson, AbelPerri, MatteoPesce-Rollins, MelissaPilia, MauraPossenti, AndreaPuccetti, SimonettaRamsey, Brian D.Rankin, JohnRoberts, OliverSgro, CarmeloSlane, PatrickSpandre, GloriaSwartz, Douglas A.Tamagawa, ToruTavecchio, FabrizioTaverna, RobertoTawara, YuzuruTennant, Allyn F.Thomas, Nicholas E.Tombesi, FrancescoTrois, AlessioTsygankov, Sergey S.Turolla, RobertoVink, JaccoWu, KinwahXie, Fei
Source
The Astrophysical Journal, 2024, 960, 3
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
Abstract
X-ray polarization is a powerful tool to investigate the geometry of accreting material around black holes, allowing independent measurements of the black hole spin and orientation of the innermost parts of the accretion disk. We perform the X-ray spectro-polarimetric analysis of an X-ray binary system in the Large Magellanic Cloud, LMC X-3, that hosts a stellar-mass black hole, known to be persistently accreting since its discovery. We report the first detection of the X-ray polarization in LMC X-3 with the Imaging X-ray Polarimetry Explorer, and find the average polarization degree of 3.2% +- 0.6% and a constant polarization angle -42 deg +- 6 deg over the 2-8 keV range. Using accompanying spectroscopic observations by NICER, NuSTAR, and the Neil Gehrels Swift observatories, we confirm previous measurements of the black hole spin via the X-ray continuum method, a ~ 0.2. From polarization analysis only, we found consistent results with low black-hole spin, with an upper limit of a < 0.7 at a 90% confidence level. A slight increase of the polarization degree with energy, similar to other black-hole X-ray binaries in the soft state, is suggested from the data but with a low statistical significance.
Comment: 14 pages, 8 figures, submitted to ApJ