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The aim of the project is to improve our current knowledge of the density of T dwarfs and the shape of the substellar initial mass function by identifying a magnitude-limited sample of T dwarfs in the full southern sky. We present the…

We present 0.9 - 2.5 um resolved spectra for the ultracool binary WISEPC J121756.91+162640.2AB. The system consists of a pair of brown dwarfs that straddles the currently defined T/Y spectral type boundary. We use synthetic spectra…

太阳与恒星天体物理 · 物理学 2015-06-17 S. K. Leggett , Michael C. Liu , Trent J. Dupuy , Caroline V. Morley , M. S. Marley , D. Saumon

We present a sample of brown dwarfs identified with the {\it Wide-field Infrared Survey Explorer} (WISE) for which we have obtained {\it Hubble Space Telescope} ({\it HST}) Wide Field Camera 3 (WFC3) near-infrared grism spectroscopy. The…

The James Webb Space Telescope (JWST) is now observing Y dwarfs, the coldest known brown dwarfs, with effective temperatures T_eff <= 475 K. The first published observations provide important information: not only is the atmospheric…

太阳与恒星天体物理 · 物理学 2023-09-27 S. K. Leggett , Pascal Tremblin

Radio detection provides unique means to measure and study magnetic fields of the coolest brown dwarfs. Previous radio surveys have observed quiescent and flaring emission from brown dwarfs down to spectral type L3.5, but only upper limits…

太阳与恒星天体物理 · 物理学 2012-02-21 Matthew Route , Alex Wolszczan

We present results of timing measurements of the binary millisecond pulsar PSR J2145-0750. Combining timing data obtained with the Effelsberg and Lovell radio telescopes we measure a significant timing parallax of 2.0(6) mas placing the…

天体物理学 · 物理学 2009-11-10 O. Loehmer , M. Kramer , T. Driebe , A. Jessner , D. Mitra , A. G. Lyne

We report on Keck optical BVRI images and spectroscopy of the companion of the binary millisecond pulsar PSR J0218+4232. A faint bluish (V=24.2, B-V=0.25) counterpart is observed at the pulsar location. Spectra of this counterpart reveal…

天体物理学 · 物理学 2011-05-23 C. G. Bassa , M. H. van Kerkwijk , S. R. Kulkarni

We report resolved near-infrared imaging and spectroscopic observations of the T8.5 binary WISEP J045853.90+643452.6AB obtained with Keck/NIRC2, Keck/OSIRIS and the Keck Laser Guide Star Adaptive Optics system. These data confirm common…

太阳与恒星天体物理 · 物理学 2015-05-30 Adam J. Burgasser , Christopher R. Gelino , Michael. C. Cushing , J. Davy Kirkpatrick

A photometric and spectroscopic analysis of 152 cool white dwarf stars is presented. The discovery of 7 new DA white dwarfs, 2 new DQ white dwarfs, 1 new magnetic white dwarf, and 3 weak magnetic white dwarf candidates, is reported, as well…

天体物理学 · 物理学 2009-10-31 P. Bergeron , S. K. Leggett , Maria Teresa Ruiz

We present preliminary non-grey model atmospheres and interiors for cool brown dwarfs. The resulting synthetic spectra are compared to available spectroscopic and photometric observations of the coolest brown dwarf yet discovered, Gl229B…

天体物理学 · 物理学 2008-02-03 France Allard , Peter H. Hauschildt , Isabelle Baraffe , Gilles Chabrier

We present the discovery of what appears to be both a uniquely cool and old white dwarf within 30 parsecs of the sun. DES J214756.46-403529.3 is detected in four separate surveys, 50 degrees away from the Galactic Plane. The combination of…

太阳与恒星天体物理 · 物理学 2021-09-28 Kevin Apps , R. L. Smart , Roberto Silvotti

We report the discovery of a wide (approximately 400 AU projected separation), common proper motion companion to the nearby M dwarf LHS 2803 (PSO J207.0300-13.7422). This object was discovered during our census of the local T dwarf…

We report on Keck and {\em Hubble Space Telescope} observations of the binary millisecond pulsar PSR B1855+09. We detect its white-dwarf companion and measure $\mv=25.90\pm0.12$ and $\mi=24.19\pm0.11$ (Vega system). From the…

天体物理学 · 物理学 2009-10-31 M. H. van Kerkwijk , J. F. Bell , V. M. Kaspi , S. R. Kulkarni

We present the first brown dwarf spectral binary characterized with JWST: WISE J014656.66+423410.0, the coldest blended-light brown dwarf binary straddling the T/Y transition. We obtained a moderate resolution (R$\sim$2700) G395H spectrum…

We present a detailed model atmosphere analysis of two of the oldest stars known in the solar neighborhood, the high proper motion white dwarfs SDSS J110217.48+411315.4 (hereafter J1102) and WD 0346+246 (hereafter WD0346). We present…

星系天体物理 · 物理学 2015-06-04 Mukremin Kilic , John R. Thorstensen , P. M. Kowalski , J. Andrews

We have carried out a search for late-type T dwarfs in the UKIDSS Galactic Plane Survey 6th Data Release. The search yielded two persuasive candidates, both of which have been confirmed as T dwarfs. The brightest, UGPS J0521+3640 has been…

Ultra-cool white dwarfs are among the oldest stellar remnants in the Universe. Their efficient gravitational settling and low effective temperatures are responsible for the smooth spectra they exhibit. For that reason, it is not possible to…

太阳与恒星天体物理 · 物理学 2020-04-08 M. C. Lam , N. C. Hambly , N. Lodieu , S. Blouin , E. J. Harvey , R. J. Smith , M. C. Galvez-Ortiz , Z. H. Zhang

We present optical and near-infrared spectroscopy of WISEA J061543.91$-$124726.8, which we rediscovered as a high motion object in the AllWISE survey. The spectra of this object are unusual; while the red optical ($\lambda >$ 7,000 \AA) and…

The Stellar Planet Survey is an ongoing astrometric search for giant planets and brown dwarfs around a sample of about 30 M-dwarfs. We have discovered several low-mass companions by measuring the motion of our target stars relative to their…

天体物理学 · 物理学 2009-11-11 Steven H. Pravdo , Stuart B. Shaklan , James Lloyd

We present two epochs of MPG/ESO 2.2m GROND simultaneous 6-band ($r'i'z'JHK$) photometric monitoring of the closest known L/T transition brown dwarf binary WISE J104915.57-531906.1AB. We report here the first resolved variability monitoring…