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The disk around the brown dwarf KPNO TAU 3
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dc.contributor.author | Broekhoven-Fiene, H. | |
dc.contributor.author | Matthews, B. | |
dc.contributor.author | Duchêne, G. | |
dc.contributor.author | Di Francesco, J. | |
dc.contributor.author | Scholz, A. | |
dc.contributor.author | Chrysostomou, A. | |
dc.contributor.author | Jayawardhana, R. | |
dc.date.accessioned | 2014-08-29T11:01:03Z | |
dc.date.available | 2014-08-29T11:01:03Z | |
dc.date.issued | 2014-07-10 | |
dc.identifier.citation | Broekhoven-Fiene , H , Matthews , B , Duchêne , G , Di Francesco , J , Scholz , A , Chrysostomou , A & Jayawardhana , R 2014 , ' The disk around the brown dwarf KPNO TAU 3 ' , Astrophysical Journal , vol. 789 , no. 2 , 155 . https://doi.org/10.1088/0004-637X/789/2/155 | en |
dc.identifier.issn | 0004-637X | |
dc.identifier.other | PURE: 144252762 | |
dc.identifier.other | PURE UUID: bb6ecf8b-9ea8-4535-966a-6634ef8d5368 | |
dc.identifier.other | Scopus: 84903317570 | |
dc.identifier.other | BibCode: 2014ApJ...789..155B | |
dc.identifier.other | WOS: 000338674900064 | |
dc.identifier.uri | https://hdl.handle.net/10023/5290 | |
dc.description | H.B.F. and B.C.M. acknowledge a Discovery Grant from the Natural Science & Engineering Research Council (NSERC) of Canada. | en |
dc.description.abstract | We present submillimeter observations of the young brown dwarfs KPNO Tau 1, KPNO Tau 3, and KPNO Tau 6 at 450 μm and 850 μm taken with the Submillimetre Common-User Bolometer Array on the James Clerk Maxwell Telescope. KPNO Tau 3 and KPNO Tau 6 have been previously identified as Class II objects hosting accretion disks, whereas KPNO Tau 1 has been identified as a Class III object and shows no evidence of circumsubstellar material. Our 3σ detection of cold dust around KPNO Tau 3 implies a total disk mass of (4.0 ± 1.1) × 10−4 M☉ (assuming a gas to dust ratio of 100:1). We place tight constraints on any disks around KPNO Tau 1 or KPNO Tau 6 of <2.1 × 10−4 M☉ and <2.7 × 10−4 M☉, respectively. Modeling the spectral energy distribution of KPNO Tau 3 and its disk suggests the disk properties (geometry, dust mass, and grain size distribution) are consistent with observations of other brown dwarf disks and low-mass T-Tauri stars. In particular, the disk-to-host mass ratio for KPNO Tau 3 is congruent with the scenario that at least some brown dwarfs form via the same mechanism as low-mass stars. | |
dc.format.extent | 6 | |
dc.language.iso | eng | |
dc.relation.ispartof | Astrophysical Journal | en |
dc.rights | © 2014. The American Astronomical Society. All rights reserved. | en |
dc.subject | Brown dwarfs | en |
dc.subject | Circumstellar matter | en |
dc.subject | Protoplanetary disks | en |
dc.subject | Stars: formation | en |
dc.subject | Stars: individual (KPNO Tau 3) | en |
dc.subject | Stars: low-mass | en |
dc.subject | QB Astronomy | en |
dc.subject.lcc | QB | en |
dc.title | The disk around the brown dwarf KPNO TAU 3 | en |
dc.type | Journal article | en |
dc.description.version | Publisher PDF | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.identifier.doi | https://doi.org/10.1088/0004-637X/789/2/155 | |
dc.description.status | Peer reviewed | en |
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