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Record W4417081433 · doi:10.48550/arxiv.2509.14556

Detection of CH3+ in the O-rich planetary nebula NGC 6302

2025· preprint· en· W4417081433 on OpenAlexafffund
Charmi Bhatt, J. Cami, E. Peeters, Nicholas Clark, Paula Moraga Baez, Kevin Volk, G. C. Sloan, Joel H. Kastner, H. L. Dinerstein, Mikako Matsuura, Bruce Balick, K. E. Kraemer, K. Justtanont, Olivia Jones, R. Sahai, Isabel Aleman, M. J. Barlow, J. Bernard‐Salas, J. A. D. L. Blommaert, Naomi Hirano, Patrick Kavanagh, F. Kemper, E. Lagadec, J. M. Laming, Frank Molster, H. Monteiro, Anita M. S. Richards, N. C. Sterling, Maryam Torki, P. A. M. van Hoof, J. R. Walsh, L. B. F. M. Waters, R. Wesson, N. J. Wright, A. A. Zijlstra

Bibliographic record

VenueResearch Explorer (The University of Manchester) · 2025
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsWestern University
FundersOffice of Naval ResearchAgencia Estatal de InvestigaciónScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaIrish Research CouncilMinisterio de Ciencia, Innovación y UniversidadesCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationScience Foundation IrelandUK Research and InnovationCanadian Space AgencyJet Propulsion LaboratorySpace Telescope Science InstituteNational Science Foundation
KeywordsPlanetary nebulaNebulaBubbleChemical processPlanetary systemStarsExcitation

Abstract

fetched live from OpenAlex

Planetary nebulae are sites where ejected stellar material evolves into complex molecules, but the precise physical conditions and chemical routes that govern these processes are unclear. The presence of abundant carbon-rich molecules in O-rich environments poses particular challenges. Here we report the first detection of methyl cation (CH3+) in any planetary nebula, observed in the O-rich nebula NGC 6302 using JWST MIRI/MRS observations. CH3+ is a key driver of organic chemistry in UV-irradiated environments. Spatially resolved observations reveal that CH3+ is co-located with 12CO, H2, H II, HCO+, and Polycyclic aromatic hydrocarbons (PAHs). LTE modelling of the CH3+ emission yields excitation temperatures of 500-800K in the inner bubble and torus, rising to 1000-2000K in the outer bubble of NGC 6302, with column densities ranging from ~10^11 to 10^13 cm^-2. This detection demonstrates that hydrocarbon radical chemistry must be incorporated into planetary nebulae chemical models. Further near-IR observations are crucial to map different chemical networks operating in these environments.

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)0.000
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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.016
Threshold uncertainty score0.031

Distilled classifier scores by category (both heads)

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)0.0010.000

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 head0.058
GPT teacher head0.287
Teacher spread0.229 · 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

Citations0
Published2025
Admission routes2
Has abstractyes

Explore more

Same venueResearch Explorer (The University of Manchester)Same topicAstrophysics and Star Formation StudiesFrench-language works237,207