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Related papers: Cool Versus Ultracool White Dwarfs

200 papers

(abridged) We report the discovery of a very cool brown dwarf, ULAS J003402.77-005206.7 (ULAS J0034-00), identified in UKIDSS DR1. We provide optical, near-infrared, and mid-infrared photometry of the source, and two near-infrared spectra.…

Although numerous white dwarf stars host dusty debris disks, the temperature distribution of these stars differs significantly from the white dwarf population as a whole. Dusty debris disks exist exclusively around white dwarfs cooler than…

Earth and Planetary Astrophysics · Physics 2021-06-09 Jordan K. Steckloff , John Debes , Amy Steele , Brandon Johnson , Elisabeth R. Adams , Seth A. Jacobson , Alessondra Springmann

We present new JHKL'M' photometry on the MKO system for a large sample of L and T dwarfs identified from SDSS and 2MASS and classified according to the scheme of Geballe et al. (2002). We have compiled a sample of 105 L and T dwarfs that…

Astrophysics · Physics 2007-05-23 D. A. Golimowski , S. K. Leggett , M. S. Marley , X. Fan. T. R. Geballe , G. R. Knapp

Using observations of Spitzer/IRAC, we report the serendipitous discovery of excess infrared emission from a single white dwarf PG 0010+280. At a temperature of 27,220 K and a cooling age of 16 Myr, it is the hottest and youngest white…

Solar and Stellar Astrophysics · Physics 2015-06-17 S. Xu , M. Jura , B. Pantoja , B. Klein , B. Zuckerman , K. Y. L. Su , H. Y. A. Meng

In recent years brown dwarfs have been extended to a new Y-dwarf class with effective temperatures colder than 500K and masses in the range 5-30 Jupiter masses. They fill a crucial gap in observable atmospheric properties between the much…

Solar and Stellar Astrophysics · Physics 2015-06-23 C. G. Tinney , Jacqueline K. Faherty , J. Davy Kirkpatrick , Mike Cushing , Caroline V. Morley , Edward L. Wright

Optical spectroscopic observations of white dwarf stars selected from catalogs based on the Gaia DR2 database reveal nine new gaseous debris disks that orbit single white dwarf stars, about a factor of two increase over the previously known…

Solar and Stellar Astrophysics · Physics 2020-12-23 Carl Melis , B. Klein , A. E. Doyle , A. J. Weinberger , B. Zuckerman , P. Dufour

We have identified eight to ten new cool white dwarfs from the Large Area Survey (LAS) Data Release 9 of the United Kingdom InfraRed Telescope (UKIRT) Infrared Deep Sky Survey (UKIDSS). The data set was paired with the Sloan Digital Sky…

Solar and Stellar Astrophysics · Physics 2014-05-02 P. -E. Tremblay , S. K. Leggett , N. Lodieu , B. Freytag , P. Bergeron , J. S. Kalirai , H. -G. Ludwig

This chapter reviews our current knowledge of metal-poor ultracool dwarfs with spectral types later than M7. The current census of M, L, and T subdwarfs is explored. The main colour trends of subdwarfs from the optical to the mid-infrared…

Solar and Stellar Astrophysics · Physics 2018-12-05 Nicolas Lodieu

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…

We report the discovery of PM J13420-3415, a faint (V=17) white dwarf with a very high proper motion mu = 2.55 arcsec/yr. The star was found in the southern sky extension of the SUPERBLINK proper motion survey. A red spectrum shows the…

Astrophysics · Physics 2009-11-13 Sebastien Lepine , R. Michael Rich , Michael M. Shara

We present YJHK photometry, or a subset, for the six Y dwarfs discovered in WISE data by Cushing et al.. The data were obtained using NIRI on the Gemini North telescope. We also present a far-red spectrum obtained using GMOS-North for…

Solar and Stellar Astrophysics · Physics 2015-06-12 S. K. Leggett , Caroline V. Morley , M. S. Marley , D. Saumon , Jonathan J. Fortney , Channon Visscher

During the low optical brightness states of AM Herculis systems (polars) when accretion has declined to a very low value, the underlying magnetic white dwarf photosphere can be modelled without the complication of thermal bremstrahlung and…

Astrophysics · Physics 2007-05-23 Edward Michael Sion

We present predictions for the surface density of ultracool dwarfs (with spectral types M8-T8) for a host of deep fields that are likely to be observed with the James Webb Space Telescope. Based on simple thin and thick/thin disk…

Astrophysics of Galaxies · Physics 2016-04-06 R. E. Ryan , I. N. Reid

We report the discovery of three nearby old halo white dwarf candidates in the Sloan Digital Sky Survey (SDSS), including two stars in a common proper motion binary system. These candidates are selected from our 2800 square degree proper…

We present photographic B, R and I photometry, and optical and near-infrared spectroscopy, of a new ultracool white dwarf (UCWD) discovered in the SuperCOSMOS Sky Survey. The spectrum of SSSJ1556-0806 shows strong flux suppression due to…

Astrophysics · Physics 2009-11-13 N. Rowell , M. Kilic , N. C. Hambly

We present an analysis of photometric, spectroscopic and spectropolarimetric data of the nearby, cool, magnetic DZ white dwarf PM J08186-3110. High dispersion spectra show the presence of Zeeman splitted spectral lines due to the presence…

Solar and Stellar Astrophysics · Physics 2020-11-11 Adela Kawka , Stéphane Vennes , Nicole F. Allard , T. Leininger , F. X. Gadéa

We describe a new survey for cool white dwarfs that supplements Sloan Digital Sky Survey photometry with USNO proper motions and follow-up spectroscopy. To date we have discovered and spectroscopically confirmed 80 new moderate temperature…

We report the discovery of a nearby, old, halo white dwarf candidate from the Sloan Digital Sky Survey. SDSS J110217.48+411315.4 has a proper motion of 1.75 arcsec/year and redder optical colors than all other known featureless (type DC)…

We present an analysis of the 0.95-14.5 micron spectral energy distributions of nine field ultracool dwarfs with spectral types ranging from L1 to T4.5. Effective temperatures, gravities, and condensate cloud sedimentation efficiencies are…

Trigonometric parallax determinations are presented for 28 late type dwarfs and brown dwarfs, including eight M dwarfs with spectral types between M7 and M9.5, 17 L dwarfs with spectral types between L0 and L8, and three T dwarfs. Broadband…

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