A Search for Disk Emission in Young Brown Dwarfs: L'-band Observations of sigma Orionis and TW Hydrae

dc.creatorJayawardhana, Ray
dc.creatorArdila, David R.
dc.creatorStelzer, Beate
dc.date2002-06-05
dc.date.accessioned2026-07-07T02:03:54Z
dc.date.available2026-07-07T02:03:54Z
dc.descriptionStudies of disks around young brown dwarfs are of paramount importance to our understanding of the origin, diversity and early evolution of sub-stellar objects. Here we present first results from a systematic search for disk emission in a spectroscopically confirmed sample of young objects near or below the sub-stellar boundary in a variety of star-forming regions. Our VLT and Keck L'-band observations of the sigma Orionis and TW Hydrae associations suggest that if a majority of brown dwarfs are born with disks, at least the inner regions of those disks evolve rapidly, possibly clearing out within a few million years.
dc.descriptionto appear in proceedings of the IAU Symposium 211 on "Brown Dwarfs", ASP Conference Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0206086
dc.identifierhttp://arxiv.org/abs/astro-ph/0206086
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4550
dc.subjectAstrophysics
dc.titleA Search for Disk Emission in Young Brown Dwarfs: L'-band Observations of sigma Orionis and TW Hydrae
dc.typetext

Files

Collections