Engineering PapersSearch

DOE OSTI · 2584677

High Optical-to-X-Ray Polarization Ratio Reveals Compton Scattering in BL Lacertae’s Jet

Agudo, Iván (ORCID:0000000237776182)·Liodakis, Ioannis (ORCID:0000000192004006)·Otero-Santos, Jorge (ORCID:0000000242415875)·Middei, Riccardo (ORCID:0000000198159092)·Marscher, Alan (ORCID:0000000173963332)·Jorstad, Svetlana (ORCID:0000000195225453)·Zhang, Haocheng (ORCID:0000000198261759)·Li, Hui [Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)] (ORCID:0000000335566568)·Di Gesu, Laura (ORCID:0000000256145028)·Romani, Roger W. (ORCID:0000000167113286)·Kim, Dawoon E. (ORCID:0000000157173736)·Fenu, Francesco (ORCID:0000000203138852)·Marshall, Herman L. (ORCID:0000000264921293)·Pacciani, Luigi (ORCID:0000000168975996)·Escudero Pedrosa, Juan (ORCID:000000024131655X)·Aceituno, Francisco José (ORCID:0000000180744760)·Agís-González, Beatriz (ORCID:0000000177028931)·Bonnoli, Giacomo (ORCID:0000000324649077)·Casanova, Víctor (ORCID:0000000320368999)·Morcuende, Daniel (ORCID:0000000194000922)·Piirola, Vilppu (ORCID:000000030186206X)·Sota, Alfredo (ORCID:0000000294046952)·Kouch, Pouya M. (ORCID:0000000293282750)·Lindfors, Elina (ORCID:0000000291556199)·McCall, Callum (ORCID:0000000233753397)·Jermak, Helen E. (ORCID:0000000211978501)·Steele, Iain A. (ORCID:0000000183975759)·Borman, George A. (ORCID:0000000272626710)·Grishina, Tatiana S. (ORCID:0000000239536676)·Hagen-Thorn, Vladimir A. (ORCID:0000000264318590)·Kopatskaya, Evgenia N. (ORCID:000000019518337X)·Larionova, Elena G. (ORCID:0000000224716500)·Morozova, Daria A. (ORCID:0000000294077804)·Savchenko, Sergey S. (ORCID:0000000341473851)·Shishkina, Ekaterina V. (ORCID:0009000224402947)·Troitskiy, Ivan S. (ORCID:0000000242180148)·Troitskaya, Yulia V. (ORCID:0000000299079876)·Vasilyev, Andrey A. (ORCID:0000000282930214)·Zhovtan, Alexey V.·Myserlis, Ioannis (ORCID:0000000330259497)·Gurwell, Mark (ORCID:0000000306853621)·Keating, Garrett (ORCID:000000023490146X)·Rao, Ramprasad (ORCID:0000000214077944)·Kang, Sincheol (ORCID:0000000201124836)·Lee, Sang-Sung (ORCID:000000026269594X)·Kim, Sanghyun (ORCID:0000000175568504)·Cheong, Whee Yeon (ORCID:0009000218715824)·Jeong, Hyeon-Woo (ORCID:0009000576298450)·Angelakis, Emmanouil (ORCID:0000000173275441)·Kraus, Alexander (ORCID:0000000241849372)·Blinov, Dmitry (ORCID:0000000306115784)·Maharana, Siddharth (ORCID:0000000270723904)·Bachev, Rumen·Jormanainen, Jenni (ORCID:0000000345197751)·Nilsson, Kari (ORCID:0000000214458683)·Fallah Ramazani, Vandad (ORCID:0000000189917744)·Casadio, Carolina (ORCID:0000000311172863)·Fuentes, Antonio (ORCID:0000000287734933)·Traianou, Efthalia (ORCID:0000000212096500)·Thum, Clemens (ORCID:0009000652926974)·Gómez, José L.·Antonelli, Lucio Angelo (ORCID:0000000250379034)·Bachetti, Matteo (ORCID:0000000245769337)·Baldini, Luca (ORCID:0000000297857726)·Baumgartner, Wayne H. (ORCID:0000000251060463)·Bellazzini, Ronaldo (ORCID:0000000224697063)·Bianchi, Stefano (ORCID:0000000246224240)·Bongiorno, Stephen D. (ORCID:0000000209012097)·Bonino, Raffaella (ORCID:0000000242641215)·Brez, Alessandro (ORCID:0000000294601821)·Bucciantini, Niccolò (ORCID:0000000288481392)·Capitanio, Fiamma (ORCID:0000000263843027)·Castellano, Simone (ORCID:0000000311114292)·Cavazzuti, Elisabetta (ORCID:0000000171509638)·Chen, Chien-Ting (ORCID:0000000249455079)·Ciprini, Stefano (ORCID:0000000207122479)·Costa, Enrico (ORCID:0000000349258523)·De Rosa, Alessandra (ORCID:0000000156686863)·Del Monte, Ettore (ORCID:0000000230136334)·Di Lalla, Niccolò (ORCID:0000000275741298)·Di Marco, Alessandro (ORCID:0000000303313259)·Donnarumma, Immacolata (ORCID:0000000247004549)·Doroshenko, Victor (ORCID:0000000181621105)·Dovčiak, Michal (ORCID:0000000300791239)·Ehlert, Steven R. (ORCID:0000000344202838)·Enoto, Teruaki (ORCID:0000000312443100)·Evangelista, Yuri (ORCID:0000000160966710)·Fabiani, Sergio (ORCID:0000000315330283)·Ferrazzoli, Riccardo (ORCID:0000000310748605)·García, Javier A. (ORCID:0000000338282448)·Gunji, Shuichi (ORCID:0000000258812445)·Hayashida, Kiyoshi·Heyl, Jeremy (ORCID:000000019739367X)·Iwakiri, Wataru (ORCID:0000000202079010)·Kaaret, Philip (ORCID:0000000236380637)·Karas, Vladimir (ORCID:0000000257600459)·Kislat, Fabian (ORCID:0000000174770380)·Kitaguchi, Takao·Kolodziejczak, Jeffery J. (ORCID:0000000201106136)·Krawczynski, Henric (ORCID:0000000210846507)

Abstract

Blazars, supermassive black hole systems with highly relativistic jets aligned with the line of sight, are the most powerful long-lived emitters of electromagnetic emission in the Universe. We report here on a radio-to-gamma-ray multiwavelength campaign on the blazar BL Lacertae with unprecedented polarimetric coverage from radio to X-ray wavelengths. The observations caught an extraordinary event on 2023 November 10–18, when the degree of linear polarization of optical synchrotron radiation reached a record value of 47.5%. In stark contrast, the Imaging X-ray Polarimetry Explorer found that the X-ray (Compton scattering or hadron-induced) emission was polarized at less than 7.4% (3 σ confidence level). We argue here that this observational result rules out a hadronic origin of the high-energy emission and strongly favors a leptonic (Compton scattering) origin, thereby breaking the degeneracy between hadronic and leptonic emission models for BL Lacertae and demonstrating the power of multiwavelength polarimetry to address this question. Furthermore, the multiwavelength flux and polarization variability, featuring an extremely prominent rise and decay of the optical polarization degree, is interpreted for the first time by the relaxation of a magnetic “spring” embedded in the newly injected plasma. This suggests that the plasma jet can maintain a predominant toroidal magnetic field component parsecs away from the central engine.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Agudo, Iván (ORCID:0000000237776182), Liodakis, Ioannis (ORCID:0000000192004006), Otero-Santos, Jorge (ORCID:0000000242415875), Middei, Riccardo (ORCID:0000000198159092), Marscher, Alan (ORCID:0000000173963332), Jorstad, Svetlana (ORCID:0000000195225453), Zhang, Haocheng (ORCID:0000000198261759), Li, Hui [Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)] (ORCID:0000000335566568), Di Gesu, Laura (ORCID:0000000256145028), Romani, Roger W. (ORCID:0000000167113286), Kim, Dawoon E. (ORCID:0000000157173736), Fenu, Francesco (ORCID:0000000203138852), Marshall, Herman L. (ORCID:0000000264921293), Pacciani, Luigi (ORCID:0000000168975996), Escudero Pedrosa, Juan (ORCID:000000024131655X), Aceituno, Francisco José (ORCID:0000000180744760), Agís-González, Beatriz (ORCID:0000000177028931), Bonnoli, Giacomo (ORCID:0000000324649077), Casanova, Víctor (ORCID:0000000320368999), Morcuende, Daniel (ORCID:0000000194000922), Piirola, Vilppu (ORCID:000000030186206X), Sota, Alfredo (ORCID:0000000294046952), Kouch, Pouya M. (ORCID:0000000293282750), Lindfors, Elina (ORCID:0000000291556199), McCall, Callum (ORCID:0000000233753397), Jermak, Helen E. (ORCID:0000000211978501), Steele, Iain A. (ORCID:0000000183975759), Borman, George A. (ORCID:0000000272626710), Grishina, Tatiana S. (ORCID:0000000239536676), Hagen-Thorn, Vladimir A. (ORCID:0000000264318590), Kopatskaya, Evgenia N. (ORCID:000000019518337X), Larionova, Elena G. (ORCID:0000000224716500), Morozova, Daria A. (ORCID:0000000294077804), Savchenko, Sergey S. (ORCID:0000000341473851), Shishkina, Ekaterina V. (ORCID:0009000224402947), Troitskiy, Ivan S. (ORCID:0000000242180148), Troitskaya, Yulia V. (ORCID:0000000299079876), Vasilyev, Andrey A. (ORCID:0000000282930214), Zhovtan, Alexey V., Myserlis, Ioannis (ORCID:0000000330259497), Gurwell, Mark (ORCID:0000000306853621), Keating, Garrett (ORCID:000000023490146X), Rao, Ramprasad (ORCID:0000000214077944), Kang, Sincheol (ORCID:0000000201124836), Lee, Sang-Sung (ORCID:000000026269594X), Kim, Sanghyun (ORCID:0000000175568504), Cheong, Whee Yeon (ORCID:0009000218715824), Jeong, Hyeon-Woo (ORCID:0009000576298450), Angelakis, Emmanouil (ORCID:0000000173275441), Kraus, Alexander (ORCID:0000000241849372), Blinov, Dmitry (ORCID:0000000306115784), Maharana, Siddharth (ORCID:0000000270723904), Bachev, Rumen, Jormanainen, Jenni (ORCID:0000000345197751), Nilsson, Kari (ORCID:0000000214458683), Fallah Ramazani, Vandad (ORCID:0000000189917744), Casadio, Carolina (ORCID:0000000311172863), Fuentes, Antonio (ORCID:0000000287734933), Traianou, Efthalia (ORCID:0000000212096500), Thum, Clemens (ORCID:0009000652926974), Gómez, José L., Antonelli, Lucio Angelo (ORCID:0000000250379034), Bachetti, Matteo (ORCID:0000000245769337), Baldini, Luca (ORCID:0000000297857726), Baumgartner, Wayne H. (ORCID:0000000251060463), Bellazzini, Ronaldo (ORCID:0000000224697063), Bianchi, Stefano (ORCID:0000000246224240), Bongiorno, Stephen D. (ORCID:0000000209012097), Bonino, Raffaella (ORCID:0000000242641215), Brez, Alessandro (ORCID:0000000294601821), Bucciantini, Niccolò (ORCID:0000000288481392), Capitanio, Fiamma (ORCID:0000000263843027), Castellano, Simone (ORCID:0000000311114292), Cavazzuti, Elisabetta (ORCID:0000000171509638), Chen, Chien-Ting (ORCID:0000000249455079), Ciprini, Stefano (ORCID:0000000207122479), Costa, Enrico (ORCID:0000000349258523), De Rosa, Alessandra (ORCID:0000000156686863), Del Monte, Ettore (ORCID:0000000230136334), Di Lalla, Niccolò (ORCID:0000000275741298), Di Marco, Alessandro (ORCID:0000000303313259), Donnarumma, Immacolata (ORCID:0000000247004549), Doroshenko, Victor (ORCID:0000000181621105), Dovčiak, Michal (ORCID:0000000300791239), Ehlert, Steven R. (ORCID:0000000344202838), Enoto, Teruaki (ORCID:0000000312443100), Evangelista, Yuri (ORCID:0000000160966710), Fabiani, Sergio (ORCID:0000000315330283), Ferrazzoli, Riccardo (ORCID:0000000310748605), García, Javier A. (ORCID:0000000338282448), Gunji, Shuichi (ORCID:0000000258812445), Hayashida, Kiyoshi, Heyl, Jeremy (ORCID:000000019739367X), Iwakiri, Wataru (ORCID:0000000202079010), Kaaret, Philip (ORCID:0000000236380637), Karas, Vladimir (ORCID:0000000257600459), Kislat, Fabian (ORCID:0000000174770380), Kitaguchi, Takao, Kolodziejczak, Jeffery J. (ORCID:0000000201106136), Krawczynski, Henric (ORCID:0000000210846507). 2025-05-16. High Optical-to-X-Ray Polarization Ratio Reveals Compton Scattering in BL Lacertae’s Jet. https://doi.org/10.3847/2041-8213%2Fadc572

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related reports

Dust Survival in Galactic Winds

This repository contains three-dimensional volumetric data from an Eulerian hydrodynamical simulation (conducted on a uniform Cartesian grid) generated by the Cholla hydrodynamics code. The datasets contain snapshots (full-grid, projections, and slices) in the HDF5 format of a multi-phase medium in which a hot, diffuse, dust-free background wind accelerates a cool, dense cloud of gas and dust. This scenario is intended to represent a supernova-driven galactic outflow, in which hot supernova winds are thought to accelerate cool interstellar medium material out of the galactic disk into the surrounding circumgalactic medium. There are three separate datasets for simulations corresponding to three cloud evolutionary scenarios: long-term cloud survival (surv), marginal cloud survival (disr), and cloud destruction (dest). Projection and slice images of the simulations are also included in this repository.

79 ASTRONOMY AND ASTROPHYSICS

Unraveling TeV halos with the Cherenkov Telescope Array

Pulsars are observed to emit bright and spatially extended gamma-ray emission at multi-TeV energies. These so-called "TeV halos" are now understood to be a nearly universal feature of middle-aged pulsars. However, many of the key physical processes that govern these systems, particularly those affecting particle diffusion, remain poorly constrained. We aim to evaluate the ability of the Cherenkov Telescope Array (CTA) to probe the physical properties of TeV halos, with a focus on the nearby and well-studied case of the Geminga pulsar. We simulate gamma-ray emission from various TeV halo models, incorporating different assumptions for the injected electron spectrum, spin-down evolution, and energy-dependent diffusion. These models are then used to forecast CTA's sensitivity to spectral and spatial differences, based on realistic mock observations and instrument response simulations. We find that CTA will be able to distinguish between a wide range of TeV halo models that are currently consistent with existing data. In particular, CTA observations can constrain the normalization, energy dependence, and spatial extent of the diffusion coefficient surrounding Geminga, as well as the spectral shape of the injected electron population.

79 ASTRONOMY AND ASTROPHYSICS