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Record W4416215234 · doi:10.1051/0004-6361/202557532

Constraining the nature of the most extreme Galactic particle accelerator

2025· article· en· W4416215234 on OpenAlexaff
A. Acharyya, F. Aharonian, Halim Ashkar, Michael Backes, R Batzofin, D. Berge, K. Bernlöhr, M. Böttcher, C. Boisson, J. Bolmont, F. Brun, B. Bruno, C. Burger-Scheidlin, T. Bylund, S. Casanova, M. Cerruti, A. Chen, M. Chernyakova, James O. Chibueze, O. Chibueze, B. Cornejo, G. Cotter, J. de Assis Scarpin, Mathieu de Bony de Lavergne, M. de Naurois, E. de Oña Wilhelmi, A.G. Delgado Giler, J. Devin, A. Djannati-Ataï, Anton Dmytriiev, K. Egberts, K. Egg, J.-P. Ernenwein, Paul Fauverge, K. Feijen, M. D. Filipović, S. Funk, S. Gabici, Y. A. Gallant, J. F. Glicenstein, Jonas Glombitza, P. Goswami, M.-H. Grondin, Lea Heckmann, B. A. Hess, J. A. Hinton, W. Hofmann, T. L. Holch, M. Holler, M. Jamrozy, F. Jankowsky, A. Jardin-Blicq, I. Jaroschewski, D. Jimeno, I. Jung-Richardt, K. Katarzyński, D. Kerszberg, B. Khélifi, Nu. Komin, K. Kosack, D. Kostunin, Rodrigo Guedes Lang, Sanja Lazarević, A. Lemière, M. Lemoine-Goumard, J.-P. Lenain, P. Liniewicz, A. Luashvili, Jonathan Mackey, D. Malyshev, V. Marandon, M.G.F. Mayer, A. K. Mehta, A. M. W. Mitchell, R. Moderski, L. Mohrmann, Alessandro Montanari, E. Moulin, J. Niemiec, Laura Olivera-Nieto, M. O. Moghadam, Sebastian Panny, R. D. Parsons, U. Pensec, Pierre Pichard, G. Pühlhofer, M. Punch, A. Quirrenbach, A. Reimer, O. Reimer, Igor Adriano de Oliveira Reis, Q. Remy, Brian Reville, Frank Rieger, G. Roellinghoff, Gavin Rowell, B. Rudak, Karim Sabri, Samar Safí-Harb, V. Sahakian, A. Santangelo, M. Sasaki, F. Schüßler, J. N. S. Shapopi, Walid Mohd Said, H. Sol, Ł. Stawarz, S. Steinmassl, T. Tanaka, A.M. Taylor, Gene Taylor, R. Terrier, Y. Tian, Anne Timmermans, M. Tsirou, Naomi Tsuji, T. Unbehaun, C. van Eldik, M. Vecchi, C. Venter, J. Vink, V. Voitsekhovskyi, S. J. Wagner, A. Wierzcholska, M. Zacharias, A. A. Zdziarski, A. Zech, W. Zhong, S. Takekawa

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of Manitoba
FundersInstitut National de Physique Nucléaire et de Physique des ParticulesNational Institutes of Natural SciencesJapan Society for the Promotion of ScienceBundesministerium für Bildung, Wissenschaft und ForschungDepartment of Science and Innovation, South AfricaUniversity of NamibiaCommissariat à l'Énergie Atomique et aux Énergies AlternativesNational Commission on Research, Science and TechnologyNational Astronomical Observatory of JapanCentre National de la Recherche ScientifiqueBundesministerium für Bildung und ForschungUniversiteit van AmsterdamAustrian Science FundMax-Planck-GesellschaftScience and Technology Facilities CouncilNational Research Foundation
KeywordsSpectral indexParticle accelerationSpectral lineFlux (metallurgy)Emission spectrumSpectral energy distributionAccelerationSpectral shape analysis

Abstract

fetched live from OpenAlex

Context. Microquasars have emerged as promising candidates to explain the cosmic-ray flux at petaelectronvolt energies. LHAASO observations revealed V4641 Sgr as the most extreme example so far. Its gamma-ray spectrum extends up to 800 TeV, which requires particles with multi-PeV energy. The TeV emission is highly extended, which challenges expectations given the reported low-inclination angle of the V4641 Sgr jets. Aims. We spatially and spectrally resolved the gamma-ray emission from V4641 Sgr and investigated the particle acceleration in the system. Methods. Using ≈100 h of H.E.S.S. data, we performed a spectro-morphological study of the gamma-ray emission around V4641 Sgr. We employed HI and dedicated CO observations of the region to infer the target material for cosmic-ray interactions. Results. We detected multi-TeV emission around V4641 Sgr with a high significance. The emission region is elongated, and its major and minor axes are 0.34° ±0.01 syst ±0.04 stat and 0.06° ±0.01 syst ±0.01 stat , respectively. We found a power-law spectrum with an index ≈1.8, and together with results from other gamma-ray instruments, this reveals a spectral energy distribution (SED) that peaks at energies of ≈100 TeV for the first time. We found indications (3 σ ) of a two-component morphology, with indistinguishable spectral properties. The position of V4641 Sgr is inconsistent with the best-fit position of the single-component model and with the dip between the two components. We found no significant evidence of an energy-dependent morphology. No dense gas was found at any distance towards V4641 Sgr, which places an upper limit of n gas ≲ 0.2 cm −3 within the gamma-ray emission region. Conclusions. The peak of the SED at ≈100 TeV identifies V4641 Sgr as a candidate cosmic-ray accelerator beyond the so-called knee. The absence of dense target gas places stringent energetic constraints on hadronic interpretations, however. The H.E.S.S. measurement requires an unusually hard (≈1.5) spectral index for the protons. A leptonic scenario faces fewer obstacles if the particle transport is fast enough to avoid losses and to reproduce the observed energy-independent morphology. The absence of bright X-ray emission across the gamma-ray emission region requires a magnetic field strength ≲3 μG, however. Our findings favour a leptonic origin of the gamma-ray emission. This conclusion does not exclude hadron acceleration in the V4641 Sgr system.

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 score0.002
Threshold uncertainty score0.004

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.001

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 head0.009
GPT teacher head0.214
Teacher spread0.205 · 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 routes1
Has abstractyes

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