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Record W4392425923 · doi:10.48550/arxiv.2403.00160

A far-ultraviolet-driven photoevaporation flow observed in a protoplanetary disk

2024· preprint· en· W4392425923 on OpenAlexfundno aff
Olivier Berné, E. Habart, E. Peeters, Ilane Schroetter, Amélie Canin, Ameek Sidhu, Ryan Chown, Émeric Bron, Thomas J. Haworth, Pamela Klaassen, Boris Trahin, Dries Van De Putte, Felipe Alarcón, Marion Zannese, A. Abergel, Edwin A. Bergin, J. Bernard‐Salas, Christiaan Boersma, J. Cami, S. Cuadrado, E. Dartois, D. Dicken, M. Elyajouri, A. Fuente, J. R. Goicoechea, Karl D. Gordon, Lina Issa, C. Joblin, Olga Kannavou, Baria Khan, Ozan Lacinbala, David Languignon, Romane Le Gal, Alexandros Maragkoudakis, Raphaël Meshaka, Yoko Okada, Takashi Onaka, Sofia Pasquini, Marc W. Pound, Massimo Robberto, M. Röllig, Bethany Schefter, Thiébaut Schirmer, Thomas Simmer, Benoît Tabone, A. G. G. M. Tielens, S. Vicente, Isabel Aleman, L. J. Allamandola, Rebecca Auchettl, G. A. Baratta, Clément Baruteau, Salma Bejaoui, Partha P. Bera, J. H. Black, F. Boulanger, Jordy Bouwman, Bernhard R. Brandl, Philippe Bréchignac, Sandra Brünken, Mridusmita Buragohain, Andrew M. Burkhardt, Alessandra Candian, S. Cazaux, J. Cernicharo, M. Chabot, Shubhadip Chakraborty, Jason Champion, Sean W. J. Colgan, Ilsa R. Cooke, A. Coutens, N. L. J. Cox, Karine Demyk, C. Engrand, Sacha Foschino, P. García-Lario, Lisseth Gavilan, Maryvonne Gérin, M. Godard, C. A. Gottlieb, P. Guillard, A. Gusdorf, Patrick Hartigan, Jinhua He, Eric Herbst, Liv Hornekær, C. Jäger, E. Janot-Pacheco, Michael J. Kaufman, F. Kemper, Sarah Kendrew, M. S. Kirsanova, Collin Knight, Sun Kwok, Á. Labiano, Thomas S. -Y. Lai, Timothy J. Lee, B. Leflóch, Franck Le Petit, Aigen Li, H. Linz, Cameron J. Mackie, S. C. Madden, Joe̋lle Mascetti, Brett A. McGuire, Pablo Merino, Elisabetta R. Micelotta, Jon A. Morse, G. Mulas, Naslim Neelamkodan, Ryou Ohsawa, R. Paladini, M. E. Palumbo, Amit Pathak, Y. J. Pendleton, Annemieke Petrignani, Thomas Pino, E. Puga, Naseem Rangwala, Mathias Rapacioli, Alessandra Ricca, Julia Román-Duval, E. Roueff, Gaël Rouillé, Farid Salama, Dinalva A. Sales, Karin Sandström, P. J. Sarre, Ella Sciamma-O’Brien, K. Sellgren, Matthew J. Shannon, A. Simonnin, S. Shenoy, D. Teyssier, Richard Thomas, Aditya Togi, L. Verstraete, Adolf N. Witt, A. Wootten, N. Ysard, Henning Zettergren, Yong Zhang, Z. Zhang, Junfeng Zhen

Bibliographic record

VenuearXiv (Cornell University) · 2024
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstro and Planetary Science
Canadian institutionsnot available
FundersAgencia Estatal de InvestigaciónScience and Engineering Research BoardJapan Society for the Promotion of ScienceScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaAmes Research CenterUnited Arab Emirates UniversityInstitut Universitaire de FranceVetenskapsrådetCentre National d’Etudes SpatialesCentre National de la Recherche ScientifiqueChinese Academy of SciencesDepartment of Science and Technology, Ministry of Science and Technology, IndiaNuclear Safety and Security CommissionDeutsche ForschungsgemeinschaftCanadian Space AgencySan José State UniversityEuropean CommissionNational Natural Science Foundation of ChinaUniversity of LeicesterNational Aeronautics and Space AdministrationNational Science Foundation
KeywordsPhotoevaporationUltravioletFar ultravioletPhysicsProtoplanetary diskAstrophysicsAstronomyPlanetOpticsSpectral line

Abstract

fetched live from OpenAlex

Most low-mass stars form in stellar clusters that also contain massive stars, which are sources of far-ultraviolet (FUV) radiation. Theoretical models predict that this FUV radiation produces photo-dissociation regions (PDRs) on the surfaces of protoplanetary disks around low-mass stars, impacting planet formation within the disks. We report JWST and Atacama Large Millimetere Array observations of a FUV-irradiated protoplanetary disk in the Orion Nebula. Emission lines are detected from the PDR; modelling their kinematics and excitation allows us to constrain the physical conditions within the gas. We quantify the mass-loss rate induced by the FUV irradiation, finding it is sufficient to remove gas from the disk in less than a million years. This is rapid enough to affect giant planet formation in the disk.

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 score0.001
Threshold uncertainty score0.004

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 head0.055
GPT teacher head0.174
Teacher spread0.118 · 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
Published2024
Admission routes1
Has abstractyes

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