UV variability and accretion in NGC 2264 Virtual Observatory Resource

Authors

1. Venuti L.
2. Bouvier J.
3. Irwin J.
4. Stauffer J.
5. Hillenbrand L.A.
6. Rebull L.,Cody A.M.
7. Alencar S.H.P.
8. Micela G.
9. Flaccomio E.
10. Peres G.

Published by

CDS

Abstract

Photometric variability is a distinctive feature of young stellar objects; exploring variability signatures at different wavelengths provides insight into the physical processes at work in these sources. We explore the variability signatures at ultraviolet (UV) and optical wavelengths for several hundred accreting and non-accreting members of the star-forming region NGC 2264 (~3Myr).

Keywords

1. accretion
2. young-stellar-objects
3. ccd-photometry
4. visible-astronomy
5. sloan-photometry
6. ultraviolet-astronomy

Bibliographic source Bibcode

2015A&A...581A..66V

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ivo://CDS.VizieR/J/A+A/581/A66

Document Object Identifer DOI

doi:10.26093/cds/vizier.35810066

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