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相关论文: A search for L dwarf binary systems

200 篇论文

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

We present the discovery of the common proper motion M9 + L0 binary DENIS J220002.05-303832.9AB, identified serendipitously with the SpeX near infrared imager/spectrograph. Spectral types are derived from resolved near infrared spectroscopy…

天体物理学 · 物理学 2009-11-11 Adam J. Burgasser , Michael W. McElwain

We present two confirmed wide separation L-dwarf common proper motion companions to nearby stars and one candidate identified from the Two Micron All Sky Survey. Spectral types from optical spectroscopy are L0 V, L2.5 V, and L8 V.…

天体物理学 · 物理学 2009-11-07 J. C. Wilson , J. Davy Kirkpatrick , J. E. Gizis , M. F. Skrutskie , D. G. Monet , J. R. Houck

We present an investigation into the rotation and stellar activity of four fully convective M dwarf `twin' wide binaries. Components in each pair have (1) astrometry confirming they are common-proper-motion binaries, (2) Gaia $BP$, $RP$,…

太阳与恒星天体物理 · 物理学 2024-12-30 Andrew A. Couperus , Todd J. Henry , Rachel A. Osten , Wei-Chun Jao , Eliot Halley Vrijmoet , Aman Kar , Elliott Horch

We present the results of an intense photometric monitoring in the near-infrared (~0.9 microns) with the TRAPPIST robotic telescope of the newly discovered binary brown dwarf WISE J104915.57-531906.1, the third closest system to the Sun at…

太阳与恒星天体物理 · 物理学 2015-06-15 M. Gillon , A. H. M. J. Triaud , E. Jehin , L. Delrez , C. Opitom , P. Magain , M. Lendl , D. Queloz

The binary brown dwarf WISE J104915.57$-$531906.1 (also Luhman 16AB), composed of a late L and early T dwarf, is a prototypical L/T transition flux reversal binary located at only 2 pc distance. Luhman 16B is a known variable whose light…

The knowledge of the binary properties of metal-poor and solar-metallicity stars can shed light on the potential differences between the formation processes responsible for both types of objects. The aim of the project is to determine the…

星系天体物理 · 物理学 2015-05-13 N. Lodieu , M. R. Zapatero Osorio , E. L. Martin

We report the discovery of LSR0602+3910, an L dwarf of class L1. The object was initially identified by Lepine et al. (2002) as a new high proper motion star lying close to the Galactic plane. Its 2MASS J-K_s=1.43 is consistent with an L…

天体物理学 · 物理学 2009-11-07 Samir Salim , Sebastien Lepine , R. Michael Rich , Michael M. Shara

I report the results of a survey for low-mass (0.030 <~ M <~ 0.013 M_solar) brown dwarfs in the direction of the TW Hya association using 2MASS. Two late-M dwarfs show signs of low surface gravity and are strong candidates to be young,…

天体物理学 · 物理学 2009-12-08 John E. Gizis

[abbreviated] We report resolved near-infrared spectroscopic monitoring of the nearby L dwarf/T dwarf binary WISE J104915.57-531906.1AB (Luhman 16AB), as part of a broader campaign to characterize the spectral energy distribution and…

We present a 20-pc, volume-limited sample of M7-L8 dwarfs created through spectroscopic follow-up of sources selected from the Two Micron All Sky Survey (2MASS) Second Incremental Release Point Source Catalog. In this paper, we present…

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…

Half of the energy emitted by late-T- and Y-type brown dwarfs emerges at 3.5 < lambda um < 5.5. We present new L' (3.43 < lambda um < 4.11) photometry obtained at the Gemini North telescope for nine late-T and Y dwarfs, and synthesize L'…

We present HST/ACS observations of 19 nearby M subdwarfs in a search for binary systems. Other than the wide common proper motion pair LHS 2140/2139, none of our sdM and esdM targets are found to be binaries. Our survey is sensitive to…

天体物理学 · 物理学 2015-05-13 Basmah Riaz , John E. Gizis , Debasmita Samaddar

The evolution of brown dwarfs from L to T spectral types is one of the least understood aspects of the ultracool population, partly for lack of a large, well-defined, and well-characterized sample in the L/T transition. To improve the…

Rotational modulations of brown dwarfs have recently provided powerful constraints on the properties of ultra-cool atmospheres, including longitudinal and vertical cloud structures and cloud evolution. Furthermore, periodic light curves…

地球与行星天体物理 · 物理学 2016-03-09 Yifan Zhou , Daniel Apai , Glenn Schneider , Mark S. Marley , Adam P. Showman

T and Y-dwarfs are among the coolest and least luminous objects detected, and they can help to understand the properties of giant planets. Their multiplicity properties can shed light on the formation process. We observed a sample six T…

太阳与恒星天体物理 · 物理学 2015-05-27 N. Huélamo , V. D. Ivanov , R. Kurtev , J. H. Girard , J. Borissova , D. Mawet , K. Muzic , C. Cáceres , C. H. F. Melo , M. F. Sterzik , D. Minniti

We report the discovery of a wide (135+/-25 AU), unusually blue L5 companion 2MASS J17114559+4028578 to the nearby M4.5 dwarf G 203-50 as a result of a targeted search for common proper motion pairs in the Sloan Digital Sky Survey and the…

天体物理学 · 物理学 2009-11-13 Jacqueline Radigan , David Lafrenière , Ray Jayawardhana , René Doyon

We report the discovery of two L dwarfs (the new spectral class defined for dwarfs cooler than the M type) in a two-epoch CCD proper motion survey of 413 square degrees, complemented by infrared photometry from DENIS. One of them has a…

天体物理学 · 物理学 2012-08-27 B. Goldman , X. Delfosse , T. Forveille , C. Afonso et al , : , the EROS collaboration

We present new infrared spectra of the T8 brown dwarf 2MASS J04151954-0935066: 2.9-4.1 micron spectra obtained with the Infrared Camera and Spectrograph on the Subaru Telescope, and 5.2-14.5 micron spectra obtained with the Infrared…