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Determining the origin of the X-ray emission in blazars through multiwavelength polarization

Title: Determining the origin of the X-ray emission in blazars through multiwavelength polarization
Authors: Liodakis, I; Zhang, H; Boula, S; Middei, R; Otero-Santos, J; Blinov, D; Agudo, I; Böttcher, M; Chen, CT; Ehlert, SR; Jorstad, SG; Kaaret, P; Krawczynski, H; Peirson, AL; Romani, RW; Tavecchio, F; Weisskopf, MC; Kouch, PM; Lindfors, E; Nilsson, K; McCall, C; Jermak, HE; Steele, IA; Myserlis, I; Gurwell, M; Keating, GK; Rao, R; Kang, S; Lee, SS; Kim, S; Cheong, WY; Jeong, HW; Angelakis, E; Kraus, A; Aceituno, FJ; Bonnoli, G; Casanova, V; Escudero, J; Agís-González, B; Morcuende, D; Sota, A; Bachev, R; Grishina, TS; Kopatskaya, EN; Larionova, EG; Morozova, DA; Savchenko, SS; Shishkina, EV; Troitskiy, IS; Troitskaya, YV; Vasilyev, AA
Publisher Information: EDP Sciences
Publication Year: 2025
Collection: Liverpool John Moores University: LJMU Research Online
Subject Terms: QB Astronomy; QC Physics
Description: The origin of the high-energy emission in astrophysical jets from black holes is a highly debated issue. This is particularly true for jets from supermassive black holes, which are among the most powerful particle accelerators in the Universe. So far, the addition of new observations and new messengers have only managed to create more questions than answers. However, the newly available X-ray polarization observations promise to finally distinguish between emission models. We use extensive multiwavelength and polarization campaigns as well as state-of-the-art polarized spectral energy distribution models to attack this problem by focusing on two X-ray polarization observations of blazar BL Lacertae in flaring and quiescent γ-ray states. We find that, regardless of the jet composition and underlying emission model, inverse-Compton scattering from relativistic electrons dominates at X-ray energies.
Document Type: article in journal/newspaper
File Description: text
Language: English
ISSN: 0004-6361
Relation: https://researchonline.ljmu.ac.uk/id/eprint/26704/1/Determining%20the%20origin%20of%20the%20Xray%20emission%20in%20blazars%20through%20multiwavelength%20polarization.pdf; Liodakis, I ORCID logoorcid:0000-0001-9200-4006 , Zhang, H ORCID logoorcid:0000-0001-9826-1759 , Boula, S ORCID logoorcid:0000-0001-7905-6928 , Middei, R, Otero-Santos, J, Blinov, D ORCID logoorcid:0000-0003-0611-5784 , Agudo, I ORCID logoorcid:0000-0002-3777-6182 , Böttcher, M ORCID logoorcid:0000-0002-8434-5692 , Chen, CT ORCID logoorcid:0000-0002-4945-5079 , Ehlert, SR ORCID logoorcid:0000-0003-4420-2838 , Jorstad, SG ORCID logoorcid:0000-0001-6158-1708 , Kaaret, P ORCID logoorcid:0000-0002-3638-0637 , Krawczynski, H ORCID logoorcid:0000-0002-1084-6507 , Peirson, AL, Romani, RW, Tavecchio, F, Weisskopf, MC, Kouch, PM ORCID logoorcid:0000-0002-9328-2750 , Lindfors, E, Nilsson, K, McCall, C ORCID logoorcid:0000-0002-3375-3397 , Jermak, HE ORCID logoorcid:0000-0002-1197-8501 , Steele, IA ORCID logoorcid:0000-0001-8397-5759 , Myserlis, I ORCID logoorcid:0000-0003-3025-9497 , Gurwell, M ORCID logoorcid:0000-0003-0685-3621 , Keating, GK ORCID logoorcid:0000-0002-3490-146X , Rao, R, Kang, S, Lee, SS ORCID logoorcid:0000-0002-6269-594X , Kim, S ORCID logoorcid:0000-0001-7556-8504 , Cheong, WY ORCID logoorcid:0009-0002-1871-5824 , Jeong, HW ORCID logoorcid:0009-0005-7629-8450 , Angelakis, E, Kraus, A ORCID logoorcid:0000-0002-4184-9372 , Aceituno, FJ ORCID logoorcid:0000-0001-8074-4760 , Bonnoli, G ORCID logoorcid:0000-0003-2464-9077 , Casanova, V, Escudero, J ORCID logoorcid:0000-0002-4131-655X , Agís-González, B, Morcuende, D, Sota, A, Bachev, R ORCID logoorcid:0000-0002-0766-864X , Grishina, TS ORCID logoorcid:0000-0002-3953-6676 , Kopatskaya, EN, Larionova, EG ORCID logoorcid:0000-0002-2471-6500 , Morozova, DA ORCID logoorcid:0000-0002-9407-7804 , Savchenko, SS ORCID logoorcid:0000-0003-4147-3851 , Shishkina, EV, Troitskiy, IS ORCID logoorcid:0000-0002-4218-0148 , Troitskaya, YV ORCID logoorcid:0000-0002-9907-9876 and Vasilyev, AA ORCID logoorcid:0000-0002-8293-0214 (2025) Determining the origin of the X-ray emission in blazars through multiwavelength polarization. Astronomy & Astrophysics, 698. ISSN 0004-6361
DOI: 10.1051/0004-6361/202554747
Availability: https://researchonline.ljmu.ac.uk/id/eprint/26704/; https://researchonline.ljmu.ac.uk/id/eprint/26704/1/Determining%20the%20origin%20of%20the%20Xray%20emission%20in%20blazars%20through%20multiwavelength%20polarization.pdf; https://doi.org/10.1051/0004-6361/202554747
Rights: cc_by
Accession Number: edsbas.23065E3F
Database: BASE