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相关论文: Discovery of a 66 mas Ultracool Binary with Laser …

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We have discovered that the extremely red, low-gravity L7 dwarf 2MASS J11193254-1137466 is a 0.14" (3.6 AU) binary using Keck laser guide star adaptive optics imaging. 2MASS J11193254-1137466 has previously been identified as a likely…

太阳与恒星天体物理 · 物理学 2017-11-10 William M. J. Best , Michael C. Liu , Trent J. Dupuy , Eugene A. Magnier

We report the discovery of a young, 0.16" binary, 2M2234+4041AB, found as the result of a Keck laser guide star adaptive optics imaging survey of young field ultracool dwarfs. Spatially resolved near-infrared photometry and spectroscopy…

We identify the L dwarf 2MASS J20261584-2943124 as an unresolved spectral binary, based on low-resolution, near-infrared spectroscopy from IRTF/SpeX. The data reveal a peculiar absorption feature at 1.6 microns, previously noted in the…

太阳与恒星天体物理 · 物理学 2015-05-19 Christopher R. Gelino , Adam J. Burgasser

(Abridged) We present multi-epoch imaging of the T5.0+T5.5 binary 2MASS J1534-2952AB obtained with the Keck laser guide star adaptive optics system. Combined with an extensive (re-)analysis of archival HST imaging, we find a total mass of…

天体物理学 · 物理学 2009-11-13 Michael C. Liu , Trent J. Dupuy , Michael J. Ireland

We report the discovery of the ultracool dwarf binary system J1250+0455AB, a low-mass (M$_\odot$$_\mathrm{tot} <$ 0.2 M$_\odot$) system in which the components straddle the M/L dwarf boundary. The binary was resolved through near-infrared…

太阳与恒星天体物理 · 物理学 2025-08-01 Sayan Baig , R. L. Smart , Hugh R. A. Jones , E. Pinna , A. Sozzetti , Gemma Cheng , Felice Cusano , Fabio Rossi , Cedric Plantet , Guido Agapito

We present the discovery and spectroscopic follow-up of a nearby late-type L dwarf (2M0614+3950), and two extremely wide very-low-mass binary systems (2M0525-7425AB and 2M1348-1344AB), resulting from our search for common proper motion…

We present updated results of a high-resolution, magnitude limited (Ks<12 mag) imaging survey of nearby low-mass M6.0-M7.5 field stars. The observations were carried out using adaptive optics at the Gemini North, VLT, Keck II, and Subaru…

天体物理学 · 物理学 2009-11-10 Nick Siegler , Laird M. Close , Kelle L. Cruz , Eduardo L. Martin , I. Neill Reid

We report the discovery of the wide L1.5+L4.5 binary 2MASS J15200224-4422419AB, identified during spectroscopic followup of high proper motion sources selected from the Two Micron All Sky Survey. This source was independently identified by…

天体物理学 · 物理学 2009-01-19 Adam J. Burgasser , Dagny L. Looper , J. Davy Kirkpatrick , Michael C. Liu

We have discovered that the brown dwarf WISEJ014656.66+423410.0 is a close binary (0.0875$\pm$0.0021 arcsec, 0.93$^{+0.12}_{-0.16}$ AU) from Keck laser guide star adaptive optics imaging. Our photometry for this system reveals that both…

太阳与恒星天体物理 · 物理学 2015-06-23 Trent J. Dupuy , Michael C. Liu , S. K. Leggett

Evidence is presented that 2MASS J03202839-0446358, a late-type dwarf with discrepant optical (M8:) and near-infrared (L1) spectral types, is an as-yet unresolved stellar/brown dwarf binary with late-type M dwarf and T dwarf components.…

天体物理学 · 物理学 2009-11-13 Adam J. Burgasser , Michael C. Liu , Michael J. Ireland , Kelle L. Cruz , Trent J. Dupuy

We present IRTF SpeX observations of the M/L binary system 2MASS J17072343-0558249. SpeX imaging resolves the system into a 1"01+/-0.17 visual binary in which both components have red near infrared colors. Resolved low-resolution (R~150)…

天体物理学 · 物理学 2008-11-26 Michael W. McElwain , Adam J. Burgasser

We present high resolution Laser Guide Star Adaptive Optics imaging of 43 late-M, L and T dwarf systems with Keck/NIRC2. These include 17 spectral binary candidates, systems whose spectra suggest the presence of a T dwarf secondary. We…

太阳与恒星天体物理 · 物理学 2015-11-11 Daniella C. Bardalez Gagliuffi , Christopher R. Gelino , Adam J. Burgasser

We present observations of a new very low mass field binary, discovered during an infrared imaging survey of 250 DENIS L and very late-M dwarfs. DENIS-J055146.0-443412.2 is an M8.5+L0 pair, with a physical separation of over 200 AU. This…

天体物理学 · 物理学 2009-11-11 M. Billeres , X. Delfosse , J. -L. Beuzit , T. Forveille , L. Marchal , E. L. Martin

Context. Though only a handful of extrasolar planets have been discovered via direct imaging, each of these discoveries had tremendous impact on our understanding of planetary formation, stellar formation and cool atmosphere physics. Aims.…

太阳与恒星天体物理 · 物理学 2016-10-05 P. Delorme , J. Gagné , J. H. Girard , A. M. Lagrange , G. Chauvin , M-E. Naud , D. Lafrenière , R. Doyon , A. Riedel , M. Bonnefoy , L. Malo

We have used the 2MASS all-sky survey and the WISE to look for ultracool dwarfs that are part of multiple systems containing main sequence stars. We cross-matched L dwarf candidates from the surveys with Hipparcos and Gliese stars, finding…

We report the identification of 2MASS J15500845+1455180 as a 0"9 L dwarf visual binary. This source is resolved in Sloan Digital Sky Survey (SDSS) images and in near-infrared imaging with the IRTF SpeX imager/spectrometer. The two…

太阳与恒星天体物理 · 物理学 2014-11-20 Adam J. Burgasser , Saurav Dhital , Andrew West

We have obtained high contrast images of four nearby, faint, and very low mass objects 2MASSJ04351455-1414468, SDSSJ044337.61+000205.1, 2MASSJ06085283-2753583 and 2MASSJ06524851-5741376 (here after 2MASS0435-14, SDSS0443+00, 2MASS0608-27…

We observe 14 young low-mass substellar objects in young moving groups using the SINFONI IFS with LGS-AO to detect and characterize 3 candidate binary systems. Together with the adopted young moving group ages we employ isochrones from…

太阳与恒星天体物理 · 物理学 2019-07-24 Per Calissendorff , Markus Janson , Rubén Asensio-Torres , Rainer Köhler

We report the discovery of a faint L6 \pm 1 companion to the previously known M9 dwarf, 2MASS J01303563-4445411, based on our near-infrared imaging and spectroscopic observations with the 3m Infrared Telescope Facility SpeX…

太阳与恒星天体物理 · 物理学 2012-02-10 Saurav Dhital , Adam J. Burgasser , Dagny L. Looper , Keivan G. Stassun

We have resolved the newly discovered T dwarf SDSS J1534+1615 into a 0.11'' binary using the Keck sodium laser guide star adaptive optics system. With an integrated-light spectral type of T3.5, this binary provides a new benchmark for…

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