International audienceWe report the first results of our ongoing campaign to discover the first brown dwarfs (BD) in NGC 2264, a young (3 Myr), populous star forming region for which our optical studies have revealed a very high density of potential candidates - 236 in <1 deg2 - from the substellar limit down to at least ~20 M_Jup for zero reddening. Candidate BD were first selected using wide field (I,z) band imaging with CFH12K, by reference to current theoretical isochrones. Subsequently, 79 (33%) of the I,z sample were found to have near-infrared 2MASS photometry (JHK_s±0.3 mag or better), yielding dereddened magnitudes and allowing further investigation by comparison with the location of NextGen and DUSTY isochrones in colour-colour an...
Deep surveys of star forming regions are the backbone of observational studies on the origin of star...
Young clusters and star forming regions are home to a large number of substellar objects with masses...
Context. Thanks to their extensive and homogeneous sky coverage, deep, large-scale, multiwavelength ...
We report the first results of our ongoing campaign to discover the first brown dwarfs (BD) in NGC 2...
NGC 2264 is a young (3 Myr), populous star forming region for which our optical studies have reveale...
We present spectroscopic follow-up observations of 68 red, faint candidates from our multi-epoch, mu...
Funding: We acknowledge support from STFC through grant number ST/R000824/1. KM acknowledges funding...
Young clusters and star forming regions are home to a large number of substellar objects with masses...
Context. The dominant formation channel of brown dwarfs (BDs) is not well constrained yet and a prom...
Context. The young star cluster near σ Orionis is one of the primary environments to study the prope...
SONYC – Substellar Objects in Nearby Young Clusters – is a survey program to investigate the frequen...
International audienceContext. Brown dwarfs represent a sizable fraction of the stellar content of o...
We have performed deep wide-field CCD photometry of the young open cluster NGC 2264 to study the ext...
Context. Star formation theories are currently divergent regarding the fundamental physical processe...
The origin of the lowest mass free-floating objects, i.e. brown dwarfs (BDs) and planetary mass obje...
Deep surveys of star forming regions are the backbone of observational studies on the origin of star...
Young clusters and star forming regions are home to a large number of substellar objects with masses...
Context. Thanks to their extensive and homogeneous sky coverage, deep, large-scale, multiwavelength ...
We report the first results of our ongoing campaign to discover the first brown dwarfs (BD) in NGC 2...
NGC 2264 is a young (3 Myr), populous star forming region for which our optical studies have reveale...
We present spectroscopic follow-up observations of 68 red, faint candidates from our multi-epoch, mu...
Funding: We acknowledge support from STFC through grant number ST/R000824/1. KM acknowledges funding...
Young clusters and star forming regions are home to a large number of substellar objects with masses...
Context. The dominant formation channel of brown dwarfs (BDs) is not well constrained yet and a prom...
Context. The young star cluster near σ Orionis is one of the primary environments to study the prope...
SONYC – Substellar Objects in Nearby Young Clusters – is a survey program to investigate the frequen...
International audienceContext. Brown dwarfs represent a sizable fraction of the stellar content of o...
We have performed deep wide-field CCD photometry of the young open cluster NGC 2264 to study the ext...
Context. Star formation theories are currently divergent regarding the fundamental physical processe...
The origin of the lowest mass free-floating objects, i.e. brown dwarfs (BDs) and planetary mass obje...
Deep surveys of star forming regions are the backbone of observational studies on the origin of star...
Young clusters and star forming regions are home to a large number of substellar objects with masses...
Context. Thanks to their extensive and homogeneous sky coverage, deep, large-scale, multiwavelength ...