NIRCAm photometric properties of ONC disks

The Orion Nebula Cluster (ONC) provides the closest example of ongoing star and planet formation in highly irradiated environments. In particular, it is a key region to study how ultraviolet (UV) radiation from massive stars can drive mass-loss in protoplanetary disks through photo-evaporation. Far-UV (FUV, energy 6

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/708/A111
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/708/A111
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/708/A111
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/708/A111
Provenance
Creator Amiot P.; Berne O.; Schroetter I.; Robberto M.; Haworth T.J.; Boersma C.,Dartois E.; Fuente A.; Goicoechea J.R.; Habart E.; McCaughrean M.J.,Onaka T.; Peeters E.
Publisher CDS
Publication Year 2026
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy