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dc.contributor.authorRiaz, Basmah
dc.contributor.authorLodieu, Nicolas
dc.contributor.authorGizis, John E.
dc.date.accessioned2011-12-14T16:01:17Z
dc.date.available2011-12-14T16:01:17Z
dc.date.issued2009-11-10
dc.identifier.citationRiaz , B , Lodieu , N & Gizis , J E 2009 , ' BROWN DWARF DISKS AT AGES OF 5-10 Myr ' , The Astrophysical Journal , vol. 705 , no. 2 , pp. 1173-1182 . https://doi.org/10.1088/0004-637X/705/2/1173
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/2299/7273
dc.description.abstractWe present Spitzer/IRAC and MIPS 24 mu m observations for 28 brown dwarfs in the Upper Scorpius (UppSco) region. We find a disk fraction of 10.7%-(+ 8.7%)(3.3%) . One object shows a small excess at 24 mu m but none at shorter wavelengths, and may be a candidate transition disk. Three objects show emission in the 10 mu m silicate feature and we present compositional fits for these sources. Flat structures are observed for all disk sources in UppSco. Also presented are the MIPS/70 mu m observations for the TW Hydrae Association brown dwarf 2MASS J1139511-315921. We discuss the structure and chemistry of brown dwarf disks at ages of similar to 5-10 Myr, and consider the possible effects of the brown dwarf densities in these clusters on the disk lifetimes.en
dc.format.extent10
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.subjectcircumstellar matter
dc.subjectopen clusters and associations: individual (Taurus, Upper Scorpius)
dc.subjectstars: low-mass, brown dwarfs
dc.subjectSCORPIUS OB ASSOCIATION
dc.subjectTW-HYDRAE-ASSOCIATION
dc.subjectLOW-MASS STARS
dc.subjectMAIN-SEQUENCE STARS
dc.subjectLARGE-AREA SEARCH
dc.subjectTAURI STARS
dc.subjectFORMING REGION
dc.subjectGRAIN-GROWTH
dc.subjectPROTOPLANETARY DISKS
dc.subjectSPITZER OBSERVATIONS
dc.titleBROWN DWARF DISKS AT AGES OF 5-10 Myren
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1088/0004-637X/705/2/1173
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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