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Irradiation origin and stability of co on trans-neptunian objects: laboratory constraints and observational evidence from JWST/DiSCo-TNOs

dc.contributor.authorHénault, E.
dc.contributor.authorBrunetto, R.
dc.contributor.authorPinilla Alonso, Noemí 
dc.contributor.author(et al.)
dc.date.accessioned2025-04-30T09:21:14Z
dc.date.available2025-04-30T09:21:14Z
dc.date.issued2025
dc.identifier.citationAstronomy and Astrophysics, 694, (2025); doi:10.1051/0004-6361/202452321
dc.identifier.issn0004-6361
dc.identifier.urihttps://hdl.handle.net/10651/78801
dc.description.sponsorshipN. P.-A. acknowledges the Ministry of Science, Innovation, and Universities (MICIU) in Spain and the State Agency for Research (AEI) for funding through the ATRAE program, project ATR2023-145683. N. P. acknowledges funding by Fundação para a Ciência e a Tecnologia (FCT) through the research grants UIDB/04434/2020 and UIDP/04434/2020.
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.rights©,
dc.sourceScopus
dc.source.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85217680328&doi=10.1051%2f0004-6361%2f202452321&partnerID=40&md5=8322569938e9860b598e4059db5fc583
dc.titleIrradiation origin and stability of co on trans-neptunian objects: laboratory constraints and observational evidence from JWST/DiSCo-TNOs
dc.typejournal article
dc.identifier.doi10.1051/0004-6361/202452321
dc.relation.publisherversionhttp://dx.doi.org/10.1051/0004-6361/202452321


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