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dc.contributor.authorRadigan, Jacqueline
dc.contributor.authorJayawardhana, Ray
dc.contributor.authorLafrenière, David
dc.contributor.authorDupuy, Trent J.
dc.contributor.authorLiu, Michael C.
dc.contributor.authorScholz, Alexander
dc.date.accessioned2014-09-25T11:31:04Z
dc.date.available2014-09-25T11:31:04Z
dc.date.issued2013-11-20
dc.identifier.citationRadigan , J , Jayawardhana , R , Lafrenière , D , Dupuy , T J , Liu , M C & Scholz , A 2013 , ' Discovery of a visual T-dwarf triple system and binarity at the L/T transition ' , Astrophysical Journal , vol. 778 , no. 1 , 36 . https://doi.org/10.1088/0004-637X/778/1/36en
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 145105583
dc.identifier.otherPURE UUID: 8fb6e5b7-4197-44fd-9389-0da23e5b2fe6
dc.identifier.otherBibCode: 2013ApJ...778...36R
dc.identifier.otherScopus: 84887592425
dc.identifier.urihttp://hdl.handle.net/10023/5496
dc.description.abstractWe present new high contrast imaging of eight L/T transition brown dwarfs (BDs) using the NIRC2 camera on the Keck II telescope. One of our targets, the T3.5 dwarf 2MASS J08381155+1511155, was resolved into a hierarchal triple with projected separations of 2.5 ± 0.5 AU and 27 ± 5 AU for the BC and A(BC) components, respectively. Resolved OSIRIS spectroscopy of the A(BC) components confirms that all system members are T dwarfs. The system therefore constitutes the first triple T-dwarf system ever reported. Using resolved photometry to model the integrated-light spectrum, we infer spectral types of T3 ± 1, T3 ± 1, and T4.5 ± 1 for the A, B, and C components, respectively. The uniformly brighter primary has a bluer J – Ks color than the next faintest component, which may reflect a sensitive dependence of the L/T transition temperature on gravity, or alternatively divergent cloud properties among components. Relying on empirical trends and evolutionary models we infer a total system mass of 0.034-0.104 M ☉ for the BC components at ages of 0.3-3 Gyr, which would imply a period of 12-21 yr assuming the system semimajor axis to be similar to its projection. We also infer differences in effective temperatures and surface gravities between components of no more than ~150 K and ~0.1 dex. Given the similar physical properties of the components, the 2M0838+15 system provides a controlled sample for constraining the relative roles of effective temperature, surface gravity, and dust clouds in the poorly understood L/T transition regime. For an age of 3 Gyr we estimate a binding energy of ~20 × 1041 erg for the wide A(BC) pair, which falls above the empirical minimum found for typical BD binaries, and suggests that the system may have been able to survive a dynamical ejection during formation. Combining our imaging survey results with previous work we find an observed binary fraction of 4/18 or 22+10-8% for unresolved spectral types of L9-T4 at separations greater than or similar to 0.''1. This translates into a volume-corrected frequency of 13+7-6%, which is similar to values of ~9%-12% reported outside the transition. Our reported L/T transition binary fraction is roughly twice as large as the binary fraction of an equivalent L9-T4 sample selected from primary rather than unresolved spectral types (6+6-4%); however, this increase is not yet statistically significant and a larger sample is required to settle the issue.
dc.format.extent16
dc.language.isoeng
dc.relation.ispartofAstrophysical Journalen
dc.rights© 2013. The American Astronomical Society. All rights reserved.en
dc.subjectBinaries: visualen
dc.subjectBrown dwarfsen
dc.subjectStars: individual: 2MASS J08381155+1511155en
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleDiscovery of a visual T-dwarf triple system and binarity at the L/T transitionen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1088/0004-637X/778/1/36
dc.description.statusPeer revieweden


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