학술논문

Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1
Document Type
Working Paper
Author
Krawczynski, HenricMuleri, FabioDovčiak, MichalVeledina, AlexandraCavero, Nicole RodriguezSvoboda, JiriIngram, AdamMatt, GiorgioGarcia, Javier A.Loktev, VladislavNegro, MichelaPoutanen, JuriKitaguchi, TakaoPodgorný, JakubRankin, JohnZhang, WendaBerdyugin, AndreiBerdyugina, Svetlana V.Bianchi, StefanoBlinov, DmitryCapitanio, FiammaDi Lalla, NiccolòDraghis, PaulFabiani, SergioKagitani, MasatoKravtsov, VadimKiehlmann, SebastianLatronico, LucaLutovinov, Alexander A.Mandarakas, NikosMarin, FrédéricMarinucci, AndreaMiller, JonMizuno, TsunefumiMolkov, Sergey V.Omodei, NicolaPetrucci, Pierre-OlivierRatheesh, AjaySakanoi, TakeshiSemena, Andrei N.Skalidis, RaphaelSoffitta, PaoloTennant, Allyn F.Thalhammer, PhillippTombesi, FrancescoWeisskopf, Martin C.Wilms, JoernZhang, SixuanAgudo, IvánAntonelli, Lucio A.Bachetti, MatteoBaldini, LucaBaumgartner, Wayne H.Bellazzini, RonaldoBongiorno, Stephen D.Bonino, RaffaellaBrez, AlessandroBucciantini, NiccolòCastellano, SimoneCavazzuti, ElisabettaCiprini, StefanoCosta, EnricoDe Rosa, AlessandraDel Monte, EttoreDi Gesu, LauraDi Marco, AlessandroDonnarumma, ImmacolataDoroshenko, VictorEhlert, Steven R.Enoto, TeruakiEvangelista, YuriFerrazzoli, RiccardoGunji, ShuichiHayashida, KiyoshiHeyl, JeremyIwakiri, WataruJorstad, Svetlana G.Karas, VladimirKolodziejczak, Jeffery J.La Monaca, FabioLiodakis, IoannisMaldera, SimoneManfreda, AlbertoMarscher, Alan P.Marshall, Herman L.Mitsuishi, IkuyukiNg, C. -Y.O'Dell, Stephen L.Oppedisano, ChiaraPapitto, AlessandroPavlov, George G.Peirson, Abel L.Perri, MatteoPesce-Rollins, MelissaPilia, MauraPossenti, AndreaPuccetti, SimonettaRamsey, Brian D.Romani, Roger W.Sgrò, CarmeloSlane, PatrickSpandre, GloriaTamagawa, ToruTavecchio, FabrizioTaverna, RobertoTawara, YuzuruThomas, Nicolas E.Trois, AlessioTsygankov, SergeyTurolla, RobertoVink, JaccoWu, KinwahXie, FeiZane, Silvia
Source
Science, Volume 378, Issue 6620, pp. 650-654 (2022)
Subject
Astrophysics - High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
Language
Abstract
A black hole x-ray binary (XRB) system forms when gas is stripped from a normal star and accretes onto a black hole, which heats the gas sufficiently to emit x-rays. We report a polarimetric observation of the XRB Cygnus X-1 using the Imaging x-ray Polarimetry Explorer. The electric field position angle aligns with the outflowing jet, indicating that the jet is launched from the inner x-ray emitting region. The polarization degree is (4.01+-0.20)% at 2 to 8 kiloelectronvolts, implying that the accretion disk is viewed closer to edge-on than the binary orbit. The observations reveal that hot x-ray emitting plasma is spatially extended in a plane perpendicular to the jet axis, not parallel to the jet.
Comment: 51 pages, 15 figures, 5 tables