MétaCan
Menu
Back to cohort
Record W4409897476 · doi:10.1038/s41550-025-02541-7

A nearby dark molecular cloud in the Local Bubble revealed via H2 fluorescence

2025· article· en· W4409897476 on OpenAlexaff
Blakesley Burkhart, T. E. Dharmawardena, Shmuel Bialy, Thomas J. Haworth, Fernando Cruz Aguirre, Young-Soo Jo, B. G. Andersson, Haeun Chung, Jerry Edelstein, I. A. Grenier, Erika Hamden, Wonyong Han, Keri Hoadley, Min-Young Lee, K. W. Min, Thomas Müller, Kate Pattle, J. E. G. Peek, Geoff Pleiss, David Schiminovich, Kwang‐Il Seon, Andrew Gordon Wilson, Catherine Zucker

Bibliographic record

VenueNature Astronomy · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of British Columbia
FundersCouncil for Higher EducationIsrael Science FoundationNational Research Foundation of KoreaMinistry of Science and ICT, South KoreaAlfred P. Sloan FoundationFlatiron HealthNuclear Safety and Security CommissionNational Research FoundationSpace Telescope Science InstituteUK Research and InnovationNational Aeronautics and Space AdministrationKorea Astronomy and Space Science InstituteKorea Advanced Institute of Science and TechnologyNational Science Foundation
KeywordsMolecular cloudAstrophysicsPhysicsSupernovaCloud computingInterstellar mediumStar formationAstronomyStarsGalaxyComputer science

Abstract

fetched live from OpenAlex

A longstanding prediction in interstellar theory posits that significant quantities of molecular gas, crucial for star formation, may be undetected due to being ’dark’ in commonly used molecular gas tracers, such as carbon monoxide. We report the discovery of Eos, a dark molecular cloud located just 94 pc from the Sun. This cloud is identified using H2 far-ultraviolet fluorescent line emission, which traces molecular gas at the boundary layers of star-forming and supernova remnant regions. The cloud edge is outlined along the high-latitude side of the North Polar Spur, a prominent X-ray/radio structure. Our distance estimate utilizes three-dimensional dust maps, the absorption of the soft-X-ray background, and hot gas tracers such as O vi; these place the cloud at a distance consistent with the Local Bubble’s surface. Using high-latitude CO maps we note a small amount ( $$M_{{{\rm{H}}}_{2}}\approx 20\text{--}40\,M_{\odot }$$ ) of CO-bright cold molecular gas, in contrast with the much larger estimate of the cloud’s true molecular mass ( $$M_{{{\rm{H}}}_{2}}\approx 3.4\times 1{0}^{3}\,M_{\odot }$$ ), indicating that most of the cloud is CO dark. Combining observational data with novel analytical models and simulations, we predict that this cloud will photoevaporate in 5.7 Myr, placing key constraints on the role of stellar feedback in shaping the closest star-forming regions to the Sun. Eos is a newly discovered molecular cloud sitting just 94 pc from the Sun. It was detected through the far-UV emission of its molecular hydrogen, having been missed in conventional molecular gas surveys due to a low abundance of common gas tracers.

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: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.868
Threshold uncertainty score0.611

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 integrity0.0000.001
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 head0.002
GPT teacher head0.230
Teacher spread0.228 · 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 designNot applicable
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

Citations8
Published2025
Admission routes1
Has abstractyes

Explore more

Same venueNature AstronomySame topicAstrophysics and Star Formation StudiesFrench-language works237,207