Mapping accretion variability in NGC 2264 Virtual Observatory Resource

Authors

1. Venuti L.
2. Bouvier J.
3. Flaccomio E.
4. Alencar S.H.P.
5. Irwin J.,Stauffer J.R.
6. Cody A.M.
7. Teixeira P.S.
8. Sousa A.P.
9. Micela G.,Cuillandre J.-C.
10. Peres G.

Published by

CDS

Abstract

Our study aims at characterizing the accretion properties of several hundred members of the star-forming region NGC 2264 (3Myr). We performed a deep u,g,r,i mapping of the cluster with CFHT/MegaCam, and monitored the simultaneous u+r variability of its members over a baseline of two weeks. Stellar parameters are determined homogeneously for about 750 monitored young objects, 40% of which are accreting T Tauri stars. Accretion properties and accretion variability are investigated and characterized from UV excess measurements. Non-accreting members of the cluster define the reference UV emission level over which flux excess is detected and measured.

Keywords

1. Open star clusters
2. Accretion
3. CCD photometry
4. Optical astronomy
5. Sloan photometry

Bibliographic source Bibcode

2014A&A...570A..82V

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/570/A82

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/570/A82

Document Object Identifer DOI

doi:10.26093/cds/vizier.35700082

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