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Record W4407788508 · doi:10.1051/0004-6361/202451334

Jetted subgalactic-size radio sources in merging galaxies

2025· article· en· W4407788508 on OpenAlexafffund
C. Stanghellini, M. Orienti, Cristiana Spingola, A. Zanichelli, D. Dallacasa, P. Cassaro, C.P. O'Dea, M-A. Perez-Torres

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicRadio Astronomy Observations and Technology
Canadian institutionsUniversity of Manitoba
FundersPlanetary Science DivisionEuropean Regional Development FundLeibniz-GemeinschaftNational Astronomical Observatories, Chinese Academy of SciencesUniversity of Illinois at Urbana-ChampaignMax-Planck-Institut für AstronomieLeibniz-Institut für Astrophysik PotsdamChina National Textile and Apparel CouncilEötvös Loránd TudományegyetemStockholms UniversitetHáskóli ÍslandsUniversitetet i OsloNatural Sciences and Engineering Research Council of CanadaDurham UniversityIstituto Nazionale di AstrofisicaAgencia Estatal de InvestigaciónScience Mission DirectorateYale UniversityUniversity of TorontoÉcole Polytechnique Fédérale de LausanneGordon and Betty Moore FoundationMinisterio de Ciencia, Innovación y UniversidadesQueen's University BelfastUniversidad Nacional Autónoma de MéxicoSpace Telescope Science InstituteLos Alamos National LaboratoryAlfred P. Sloan FoundationJohns Hopkins UniversityHarvard UniversityQueen's UniversityOhio State UniversityCalifornia Institute of TechnologyUniversity of Colorado BoulderTurun YliopistoAarhus UniversitetCarnegie Institution of WashingtonNational Central UniversitySmithsonian Astrophysical ObservatoryFlatiron HealthSmithsonian InstitutionNational Aeronautics and Space AdministrationNanjing UniversityNew Mexico State UniversityYunnan UniversityNational Science Foundation
KeywordsPhysicsAstrophysicsRadio galaxyX-shaped radio galaxyGalaxyJet (fluid)AstronomyAstrophysical jetActive galactic nucleus

Abstract

fetched live from OpenAlex

Context. The long-standing question concerning jetted subgalactic-size (JSS) radio sources is whether they will evolve into large radio galaxies, die before escaping the host galaxy, or remain indefinitely confined to their compact size. Aims. Our main goal is to propose a scenario that explains the relative number of JSS radio sources and their general properties. Methods. We studied the parsec-scale radio morphology of a complete sample of 21 objects using Very Long Baseline Array (VLBA) observations at various frequencies and analyzed the morphological characteristics of their optical hosts. Results. Many of these radio sources exhibit radio morphologies consistent with transverse motions of their bright edges and are found in dynamically disturbed galaxies. VLBA images suggest the possible presence of large-angle, short-period precessing jets, and an orbital motion of the radio-loud active galactic nucleus (AGN) in a dual or binary system. The majority of JSS radio sources appear to be in systems in different stages of their merging evolution. Conclusions. We propose a scenario where rapid jet redirection, through precession or orbital motion, prevents the jet from penetrating the interstellar medium (ISM) sufficiently to escape the host galaxy. Most JSS radio sources remain compact due to their occurrence in merging galaxies.

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 machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.001
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.001
Threshold uncertainty score0.005

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.001
Scholarly communication0.0010.001
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.005
GPT teacher head0.205
Teacher spread0.200 · 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 source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
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

Citations4
Published2025
Admission routes2
Has abstractyes

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