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Record W4403915467 · doi:10.1051/0004-6361/202452311

A wiggling filamentary jet at the origin of the blazar multi-wavelength behaviour

2024· article· en· W4403915467 on OpenAlexaff
C. M. Raiteri, M. Villata, M. I. Carnerero, S. O. Kurtanidze, D. O. Mirzaqulov, E. Benítez, G. Bonnoli, D. Carosati, J. A. Acosta‐Pulido, I. Agudo, T. S. Andreeva, G. Apolonio, R. Bachev, Г. А. Борман, V. Bozhilov, L. F. Brown, W. Carbonell, C. Casadio, Wen-Ping Chen, G. Damljanović, Sh. A. Ehgamberdiev, D. Elsäesser, Juan Escudero, M. Feige, Antonio Fuentes, D. Gabellini, K. Gazeas, M. Giroletti, T. S. Grishina, Alok C. Gupta, Mark Gurwell, Gamal M. Hamed, D. Hiriart, M. W. Hodges, R. Z. Ivanidze, M. D. Joner, Svetlana G. Jorstad, S. Kiehlmann, G. N. Kimeridze, E. N. Kopatskaya, Yu. A. Kovalev, Y.Y. Kovalev, O. M. Kurtanidze, A. Kurtenkov, Е. Г. Ларионова, A. Lessing, H. C. Lin, J. López, C. Lorey, J. Ludwig, N. Marchili, Alessandro Marchini, Alan P. Marscher, Katsura Matsumoto, W. Max-Moerbeck, B. Mihov, M. Minev, М. Г. Мингалиев, A. Modaressi, D. A. Morozova, F. Mortari, T.V. Mufakharov, I. Myserlis, M. G. Nikolashvili, T. J. Pearson, A.V. Popkov, I. A. Rahimov, A. C. S. Readhead, David Reinhart, R. Reeves, S. Righini, F. D. Romanov, С. С. Савченко, E. Semkov, L. A. Sigua, L. Slavcheva-Mihova, Yu. V. Sotnikova, R. Steineke, M. Stojanović, A. Strigachev, A. Takey, Efthalia Traianou, Yu. V. Troitskaya, I. S. Troitskiy, An-Li Tsai, A. Valcheva, A. A. Vasilyev, G. Verna, O. Vince, K. Vrontaki, Z. R. Weaver, Q. Yuldoshev, E. Zaharieva, А. В. Жовтан

Bibliographic record

VenueAstronomy and Astrophysics · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsSaint Mary's UniversityAbbey Ridge Observatory
FundersFP7 Research Potential of Convergence RegionsDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoInstituto de Astrofísica de CanariasInstituto de Astrofísica de AndalucíaSerbian Academy of Sciences and ArtsNational and Kapodistrian University of AthensIstituto Nazionale di AstrofisicaCentre National de la Recherche ScientifiqueAgencia Estatal de InvestigaciónUniversity of CreteNational Central UniversityNuclear Safety and Security CommissionSmithsonian Astrophysical ObservatoryBulgarian National Science FundNational Research Institute of Astronomy and GeophysicsRegione Autonoma della SardegnaCalifornia Institute of TechnologyEuropean CommissionAcademia SinicaBrigham Young UniversityNational Aeronautics and Space AdministrationMinistry of Science and Higher Education of the Russian FederationJapan Society for the Promotion of ScienceScience and Technology Development FundMax-Planck-GesellschaftSmithsonian InstitutionJunta de AndalucíaNational Science Foundation
KeywordsPhysicsBlazarAstrophysicsJet (fluid)WavelengthAstronomyOpticsMechanics

Abstract

fetched live from OpenAlex

Context. Blazars are beamed active galactic nuclei (AGNs) known for their strong multi-wavelength variability on timescales ranging from years down to minutes. Many different models have been proposed to explain this variability. Aims. We aim to investigate the suitability of the twisting jet model presented in previous works to explain the multi-wavelength behaviour of BL Lacertae, the prototype of one of the blazar classes. According to this model, the jet is inhomogeneous, curved, and twisting, and the long-term variability is due to changes in the Doppler factor due to variations in the orientation of the jet-emitting regions. Methods. We analysed optical data of the source obtained during monitoring campaigns organised by the Whole Earth Blazar Telescope (WEBT) in 2019–2022, together with radio data from the WEBT and other teams, and γ -ray data from the Fermi satellite. In this period, BL Lacertae underwent an extraordinary activity phase, reaching its historical optical and γ -ray brightness maxima. Results. The application of the twisting jet model to the source light curves allows us to infer the wiggling motion of the optical, radio, and γ -ray jet-emitting regions. The optical-radio correlation shows that the changes in the radio viewing angle follow those in the optical viewing angle by about 120 days, and it suggests that the jet is composed of plasma filaments, which is in agreement with some radio high-resolution observations of other sources. The γ -ray emitting region is found to be co-spatial with the optical one, and the analysis of the γ -optical correlation is consistent with both the geometric interpretation and a synchrotron self-Compton (SSC) origin of the high-energy photons. Conclusions. We propose a geometric scenario where the jet is made up of a pair of emitting plasma filaments in a sort of double-helix curved rotating structure, whose wiggling motion produces changes in the Doppler beaming and can thus explain the observed multi-wavelength long-term variability.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Other design · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.894
Threshold uncertainty score0.777

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.011
GPT teacher head0.224
Teacher spread0.213 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designOther design
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations11
Published2024
Admission routes1
Has abstractyes

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