Add to ORKGWe present homogeneous multi-band (optical+UV) photometry (table2) and stellar parameters (table3: accreting/non-accreting status, spectral type, Av, bolometric luminosity, stellar mass, stellar radius and age estimate) for 757 young stars in the cluster (706 confirmed members + 51 newly identified candidates from our survey). In table4, we present the UV excess measurements, u-band excess luminosity, median accretion rates and their measured variability ranges for 237 accreting objects in our sample. (3 data files)
Photoelectric UBV magnitudes and colours have been determined for 138 stars in NGC 2264, having memb...
Context. Space photometric time series of the most massive members of the young open cluster NGC 226...
Variability is a signature feature of young stars. Among the well known light curve phenomena are pe...
Context. The accretion process has a central role in the formation of stars and planets.Aims. We aim...
Context. The accretion process has a central role in the formation of stars and planets. ...
Context. Photometric variability is a distinctive feature of young stellar objects; exploring variab...
Based on more than four weeks of continuous high cadence photometric monitoring of several hundred m...
Context. The accretion process has a central role in the formation of stars and planets. Aims. We ai...
We have performed deep wide-field CCD photometry of the young open cluster NGC 2264 to study the ext...
Context. The accretion process has a central role in the formation of stars and planets. Aims. We...
Context. NGC 2264 is a young cluster whose accretion properties can be investigated in detail by tak...
© 2017 ESO. Context. Space photometric time series of the most massive members of the young open clu...
VBLUW photometry of 112 stars with V <13 in the area of the very young cluster NGC 2264, is prese...
X-ray properties of sources in the Chandra observations of NGC6231 (columns 1-13), and their identif...
Context. NGC 2264 is a young cluster whose accretion properties can be investigated in detail by tak...
Photoelectric UBV magnitudes and colours have been determined for 138 stars in NGC 2264, having memb...
Context. Space photometric time series of the most massive members of the young open cluster NGC 226...
Variability is a signature feature of young stars. Among the well known light curve phenomena are pe...
Context. The accretion process has a central role in the formation of stars and planets.Aims. We aim...
Context. The accretion process has a central role in the formation of stars and planets. ...
Context. Photometric variability is a distinctive feature of young stellar objects; exploring variab...
Based on more than four weeks of continuous high cadence photometric monitoring of several hundred m...
Context. The accretion process has a central role in the formation of stars and planets. Aims. We ai...
We have performed deep wide-field CCD photometry of the young open cluster NGC 2264 to study the ext...
Context. The accretion process has a central role in the formation of stars and planets. Aims. We...
Context. NGC 2264 is a young cluster whose accretion properties can be investigated in detail by tak...
© 2017 ESO. Context. Space photometric time series of the most massive members of the young open clu...
VBLUW photometry of 112 stars with V <13 in the area of the very young cluster NGC 2264, is prese...
X-ray properties of sources in the Chandra observations of NGC6231 (columns 1-13), and their identif...
Context. NGC 2264 is a young cluster whose accretion properties can be investigated in detail by tak...
Photoelectric UBV magnitudes and colours have been determined for 138 stars in NGC 2264, having memb...
Context. Space photometric time series of the most massive members of the young open cluster NGC 226...
Variability is a signature feature of young stars. Among the well known light curve phenomena are pe...