학술논문

X-ray Polarization Observations of BL Lacertae
Document Type
Working Paper
Author
Middei, RiccardoLiodakis, IoannisPerri, MatteoPuccetti, SimonettaCavazzuti, ElisabettaDi Gesu, LauraEhlert, Steven R.Madejski, GrzegorzMarscher, Alan P.Marshall, Herman L.Muleri, FabioNegro, MichelaJorstad, Svetlana G.Agís-González, BeatrizAgudo, IvánBonnoli, GiacomoBernardos, Maria I.Casanova, VíctorGarcía-Comas, MayaHusillos, CésarMarchini, AlessandroSota, AlfredoKouch, Pouya M.Borman, George A.Kopatskaya, Evgenia N.Larionova, Elena G.Morozova, Daria A.Savchenko, Sergey S.Vasilyev, Andrey A.Zhovtan, Alexey V.Casadio, CarolinaEscudero, JuanMyserlis, IoannisHales, AntonioKameno, SeijiKneissl, RuedigerMessias, HugoNagai, HiroshiBlinov, DmitryBourbah, Ioakeim G.Kiehlmann, SebastianKontopodis, EvangelosMandarakas, NikosRomanopoulos, StylianosSkalidis, RaphaelVervelaki, AnnaMasiero, Joseph R.Mawet, DimitriMillar-Blanchaer, Maxwell A.Panopoulou, Georgia V.Tinyanont, SamapornBerdyugin, Andrei V.Kagitani, MasatoKravtsov, VadimSakanoi, TakeshiImazawa, RyoSasada, MahitoFukazawa, YasushiKawabata, Koji S.Uemura, MakotoMizuno, TsunefumiNakaoka, TatsuyaAkitaya, HiroshiGurwell, MarkRao, RamprasadDi Lalla, NiccolóCibrario, NicolóDonnarumma, ImmacolataKim, Dawoon E.Omodei, NicolaPacciani, LuigiPoutanen, JuriTavecchio, FabrizioAntonelli, Lucio A.Bachetti, MatteoBaldini, LucaBaumgartner, Wayne H.Bellazzini, RonaldoBianchi, StefanoBongiorno, Stephen D.Bonino, RaffaellaBrez, AlessandroBucciantini, NiccolóCapitanio, FiammaCastellano, SimoneCiprini, StefanoCosta, EnricoDe Rosa, AlessandraDel Monte, EttoreDi Marco, AlessandroDoroshenko, VictorDovčiak, MichalEnoto, TeruakiEvangelista, YuriFabiani, SergioFerrazzoli, RiccardoGarcia, Javier A.Gunji, ShuichiHayashida, KiyoshiHeyl, JeremyIwakiri, WataruKaras, VladimirKitaguchi, TakaoKolodziejczak, Jeffery J.Krawczynski, HenricLa Monaca, FabioLatronico, LucaMaldera, SimoneManfreda, AlbertoMarin, FrédéricMarinucci, AndreaMassaro, FrancescoMatt, GiorgioMitsuishi, IkuyukiNg, C. -Y.O'Dell, Stephen L.Oppedisano, ChiaraPapitto, AlessandroPavlov, George G.Peirson, Abel L.Pesce-Rollins, MelissaPetrucci, Pierre-OlivierPilia, MauraPossenti, AndreaRamsey, Brian D.Rankin, JohnRatheesh, AjayRomani, Roger W.Sgró, CarmeloSlane, PatrickSoffitta, PaoloSpandre, GloriaTamagawa, ToruTaverna, RobertoTawara, YuzuruTennant, Allyn F.Thomas, Nicholas E.Tombesi, FrancescoTrois, AlessioTsygankov, SergeyTurolla, RobertoVink, JaccoWeisskopf, Martin C.Wu, KinwahXie, FeiZane, Silvia
Source
2023, ApJ Letters, 942, L10
Subject
Astrophysics - High Energy Astrophysical Phenomena
Astrophysics - Astrophysics of Galaxies
Language
Abstract
Blazars are a class of jet-dominated active galactic nuclei with a typical double-humped spectral energy distribution. It is of common consensus the Synchrotron emission to be responsible for the low frequency peak, while the origin of the high frequency hump is still debated. The analysis of X-rays and their polarization can provide a valuable tool to understand the physical mechanisms responsible for the origin of high-energy emission of blazars. We report the first observations of BL Lacertae performed with the Imaging X-ray Polarimetry Explorer ({IXPE}), from which an upper limit to the polarization degree $\Pi_X<$12.6\% was found in the 2-8 keV band. We contemporaneously measured the polarization in radio, infrared, and optical wavelengths. Our multiwavelength polarization analysis disfavors a significant contribution of proton synchrotron radiation to the X-ray emission at these epochs. Instead, it supports a leptonic origin for the X-ray emission in BL Lac.
Comment: 17 pages, 5 figures, accepted for publication in ApJL