A deep, wide-field search for substellar members in NGC 2264
arXiv:astro-ph/0501636 · doi:10.1051/0004-6361:20042164
Abstract
We 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 deg - from the substellar limit down to at least 20 M for zero reddening. Candidate BD were first selected using wide field () band imaging with CFH12K, by reference to current theoretical isochrones. Subsequently, 79 (33%) of the sample were found to have near-infrared 2MASS photometry ( 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 and colour-magnitude diagrams involving various combinations of ,, and . We discuss the status and potential substellarity of a number of relatively unreddened (A 5) likely low-mass members in our sample, but in spite of the depth of our observations in , we are as yet unable to unambiguously identify substellar candidates using only 2MASS data. Nevertheless, there are excellent arguments for considering two faint (observed 18.4 and 21.2) objects as cluster candidates with masses respectively at or rather below the hydrogen burning limit. More current candidates could be proven to be cluster members with masses around 0.1 M {\it via} gravity-sensitive spectroscopy, and deeper near-infrared imaging will surely reveal a hitherto unknown population of young brown dwarfs in this region, accessible to the next generation of deep near-infrared surveys.
arXiv comment10 pages, 12 figures, accepted by A&A
References in corpus (20)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- Galactic Stellar and Substellar Initial Mass Function
- Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 20945
- Evolutionary models for very-low-mass stars and brown dwarfs with dusty atmospheres
- The Stellar IMF from Turbulent Fragmentation
- The Formation of a Star Cluster: Predicting the Properties of Stars and Brown Dwarfs
- Sixty-seven Additional L Dwarfs Discovered by the Two Micron All Sky Survey (2MASS)
- The Formation of Brown Dwarfs as Ejected Stellar Embryos
- Meeting the Cool New Neighbors V: A 2MASS-Selected Sample of Ultracool Dwarfs
- Infrared Spectroscopy of Substellar Objects in Orion
- New Low-Mass Members of the Taurus Star-Forming Region
- A rotational and variability study of a large sample of PMS stars in NGC 2264
- The Substellar Mass Function in sigma Orionis
- Brown dwarfs in the Pleiades cluster : clues to the substellar mass function
- Infrared Colors at the Stellar/Substellar Boundary
- The Galactic disk mass-budget : II. Brown dwarf mass-function and density
- Four Brown Dwarfs in the Taurus Star-Forming Region
- Spectroscopic identification of DENIS-selected brown dwarf candidates in the Upper Scorpius OB association
- Photometric variability of young brown dwarfs in the sigma Orionis open cluster
- Kinematics of stars and brown dwarfs at birth