6533b882fe1ef96bd12d9d82
RESEARCH PRODUCT
UV variability and accretion in NGC 2264
L. VenutiJ. BouvierJ. IrwinJ. StaufferL.a. HillenbrandL. RebullA.m. Cody Alencar S.h.p.G. MicelaE. FlaccomioG. Peressubject
interstellar mediumAccretionUltraviolet astronomyAstrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstellar astronomyYoung stellar objectsOptical astronomyPhotometryobservational astronomyAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsCCD photometryAstrophysical ProcessesNatural SciencesSloan photometryAstrophysics::Galaxy Astrophysicsdescription
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). Cone search capability for table J/A+A/581/A66/table2 (Median photometry, variability amplitudes, light curve rms, J index, and color slopes for members monitored at CFHT)
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2015-01-01 |