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Related papers: Kelu-1 is a Binary L Dwarf: First Brown Dwarf Scie…

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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.…

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…

Astrophysics of Galaxies · Physics 2015-05-13 N. Lodieu , M. R. Zapatero Osorio , E. L. Martin

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.…

Despite their key role in astrophysics, the binary properties of RR Lyrae stars (RRL) remain almost completely unknown since only a single RRL is confirmed as belonging to a binary system. Finding companions to RRL is difficult since most…

We present multi-colour photometry of four field ultracool dwarfs with the triple-beam photometer ultracam. Data were obtained simultaneously in the Sloan-g' band and a specially designed narrow-band NaI filter. The previously reported…

Astrophysics · Physics 2009-11-11 S. P. Littlefair , V. S. Dhillon , T. R. Marsh , T. Shahbaz , E. L. Martin

We present VLT/SINFONI J, H+K spectra of seven close visual pairs in M dwarf binary/triple systems, discovered or observed by the AstraLux M dwarf survey. We determine the spectral types to within 1.0 subclasses from comparison to template…

Solar and Stellar Astrophysics · Physics 2016-01-27 C. Bergfors , W. Brandner , M. Bonnefoy , J. Schlieder , M. Janson , Th. Henning , G. Chauvin

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…

Astrophysics · Physics 2009-11-13 Jacqueline Radigan , David Lafrenière , Ray Jayawardhana , René Doyon

We present the first results from our high-precision infrared (IR) astrometry program at the Canada-France-Hawaii Telescope. We measure parallaxes for 83 ultracool dwarfs (spectral types M6--T9) in 49 systems, with a median uncertainty of…

Solar and Stellar Astrophysics · Physics 2015-06-03 Trent J. Dupuy , Michael C. Liu

We present analyses of high resolution and medium resolution spectra of early L dwarfs. We used our latest set of model atmospheres to reproduce and analyze the observed features. We can model the optical flux and the atomic line profiles…

An unresolved, likely L dwarf companion to the DA white dwarf GD1400 is reported. This would be only the second such system known, discovered 17 years after the prototype L dwarf, GD165B, was determined to be a companion to a white dwarf.…

Astrophysics · Physics 2009-11-10 J. Farihi , M. Christopher

We present a sequence of high resolution (R~20,000 or 15 km/s) infrared spectra of stars and brown dwarfs spanning spectral types M2.5 to T6. Observations of 16 objects were obtained using eight echelle orders to cover part of the J-band…

We present the serendipitous discovery of an L subdwarf, 2MASS J06164006-6407194, in a search of the Two Micron All Sky Survey for T dwarfs. Its spectrum exhibits features indicative of both a cool and metal poor atmosphere including a…

Solar and Stellar Astrophysics · Physics 2014-11-18 M. C. Cushing , D. Looper , A. J. Burgasser , J. D. Kirkpatrick , J. Faherty , K. Cruz , A. Sweet , R. E. Sanderson

Brown dwarfs at the L-T transition likely experience an inhomogeneous clearing of the clouds in their atmospheres. The resulting surface of thin and thick cloudy patches has been put forward to explain the observed variability, J-band…

Earth and Planetary Astrophysics · Physics 2025-04-30 S. de Regt , I. A. G. Snellen , N. F. Allard , D. González Picos , S. Gandhi , N. Grasser , R. Landman , P. Mollière , E. Nasedkin , T. Stolker , Y. Zhang

We present Keck II adaptive optics near infrared imaging and spectroscopic observations of the central regions of the powerful radio galaxy Cygnus A. The 0.05" resolution images clearly show an unresolved nucleus between two spectacular…

Astrophysics · Physics 2009-11-10 Gabriela Canalizo , Claire Max , David Whysong , Robert Antonucci , Scott E. Dahm

We report the discovery of twenty-one hitherto unknown bright southern ultracool dwarfs with spectral types in the range M7 to L5.5, together with new observations of a further three late M dwarfs previously confirmed. Three more objects…

This paper describes the discovery of seven dwarf objects of spectral type `L' (objects cooler than the latest M dwarfs) in commissioning imaging data taken by the Sloan Digital Sky Survey (SDSS). Low-resolution spectroscopy shows that…

Astrophysics · Physics 2009-10-31 SDSS Collaboration , Xiaohui Fan

Optical and near-infrared spectroscopy of the newly discovered peculiar L dwarf 2MASS J11263991-5003550 are presented. Folkes et al. identified this source as a high proper motion L9+/-1 dwarf based on its strong H2O absorption at 1.4…

We have used Pan-STARRS1 to discover an extremely red late-L dwarf, which has (J-K)_MKO = 2.84 and (J-K)_2MASS = 2.78, making it the reddest known field dwarf and second only to 2MASS J1207-39b among substellar companions. Near-IR…

We report the discovery of a peculiar L dwarf from the UKIDSS LAS, ULAS J222711-004547. The very red infrared photometry (MKO J-K = 2.79$\pm$0.06, WISE W1-W2 = 0.65$\pm$0.05) of ULAS J222711-004547 makes it one of the reddest brown dwarfs…

Solar and Stellar Astrophysics · Physics 2014-03-05 F. Marocco , A. C. Day-Jones , P. W. Lucas , H. R. A. Jones , R. L. Smart , Z. H. Zhang , J. I. Gomes , B. Burningham , D. J. Pinfield , R. Raddi , L. Smith

We present the analysis of high resolution follow-up observations of OGLE-2016-BLG-1195 using Laser Guide Star Adaptive Optics with Keck, seven years after the event's peak. We resolve the lens, measuring its flux and the relative…

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