Accretion process in NGC 2264

DOI

NGC 2264 is a young stellar cluster (~3Myr) with hundreds of low-mass accreting stars that allow a detailed analysis of the accretion process taking place in the pre-main sequence. Our goal is to relate the photometric and spectroscopic variability of classical T Tauri stars to the physical processes acting in the stellar and circumstellar environment, within a few stellar radii from the star. NGC 2264 was the target of a multiwavelength observational campaign with CoRoT, MOST, Spitzer, and Chandra satellites and photometric and spectroscopic observations from the ground. We classified the CoRoT light curves of accreting systems according to their morphology and compared our classification to several accretion diagnostics and disk parameters.

Cone search capability for table J/A+A/586/A47/table2 (Parameters of the CTTSs observed by CoRoT and/or FLAMES/VLT)

Cone search capability for table J/A+A/586/A47/table3 (Parameters of the WTTSs observed by CoRoT and/or FLAMES/VLT)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35860047
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/586/A47
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/586/A47
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/586/A47
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/586/A47
Provenance
Creator Sousa A.P.; Alencar S.H.P.; Bouvier J.; Stauffer J.R.; Venuti L.; Flaccomio E.; Hillenbrand L.; Cody A.M.; Teixeira P.S.; Guimaraes M.M.; McGinnis P.T.; Rebull L.; Fueresz G.; Micela G.; Gameiro J.F.
Publisher CDS
Publication Year 2016
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; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy