Results 1 to 10 of about 69,461 (285)

The First JWST Spectral Energy Distribution of a Y Dwarf [PDF]

open access: goldThe Astrophysical Journal Letters, 2023
We present the first JWST spectral energy distribution of a Y dwarf. This spectral energy distribution of the Y0 dwarf WISE J035934.06−540154.6 consists of low-resolution ( λ /Δ λ ∼100) spectroscopy from 1–12 μ m and three photometric points at 15, 18 ...
Samuel A. Beiler   +5 more
doaj   +5 more sources

WATER CLOUDS IN Y DWARFS AND EXOPLANETS [PDF]

open access: greenThe Astrophysical Journal, 2014
The formation of clouds affects brown dwarf and planetary atmospheres of nearly all effective temperatures. Iron and silicate condense in L dwarf atmospheres and dissipate at the L/T transition.
Caroline Morley   +6 more
core   +8 more sources

JWST/NIRCam Discovery of the First Y+Y Brown Dwarf Binary: WISE J033605.05–014350.4 [PDF]

open access: goldThe Astrophysical Journal Letters, 2023
We report the discovery of the first brown dwarf binary system with a Y dwarf primary, WISE J033605.05−014350.4, observed with NIRCam on JWST with the F150W and F480M filters.
Per Calissendorff   +27 more
doaj   +5 more sources

Outstanding Issues in Our Understanding of L, T, and Y Dwarfs [PDF]

open access: green, 2007
Since the discovery of the first L dwarf 19 years ago and the discovery of the first T dwarf 7 years after that, we have amassed a large list of these objects, now numbering almost six hundred.
J. Davy Kirkpatrick
core   +7 more sources

JWST 1.5 μm and 4.8 μm Photometry of Y Dwarfs

open access: goldThe Astronomical Journal
Brown dwarfs lack nuclear fusion and cool with time; the coldest known have an effective temperature below 500 K, and are known as Y dwarfs. We present a James Webb Space Telescope (JWST) photometric data set of Y dwarfs: 23 were imaged in wide-field ...
Loïc Albert   +22 more
doaj   +3 more sources

TWO EXTRAORDINARY SUBSTELLAR BINARIES AT THE T/Y TRANSITION AND THEY-BAND FLUXES OF THE COOLEST BROWN DWARFS, [PDF]

open access: greenThe Astrophysical Journal, 2012
Using Keck laser guide star adaptive optics imaging, we have found that the T9 dwarf WISE J1217+1626 and T8 dwarf WISE J1711+3500 are exceptional binaries, with unusually wide separations (~0.8 arcsec, 8-15 AU), large near-IR flux ratios (~2-3 mags), and
Michael C. Liu   +4 more
core   +6 more sources

Astrometry and Photometry for ≈1000 L, T, and Y Dwarfs from the UKIRT Hemisphere Survey [PDF]

open access: goldThe Astronomical Journal, 2023
We present the positions, proper motions, and near-infrared photometry for 966 known objects with spectral types later than M that were observed as part of the the UKIRT Hemisphere Survey (UHS).
Adam C. Schneider   +7 more
doaj   +2 more sources

High-precision Atmospheric Characterization of a Y Dwarf with JWST NIRSpec G395H Spectroscopy: Isotopologue, C/O Ratio, Metallicity, and the Abundances of Six Molecular Species [PDF]

open access: goldThe Astronomical Journal
The launch of the James Webb Space Telescope (JWST) marks a pivotal moment for precise atmospheric characterization of Y dwarfs, the coldest brown dwarf spectral type.
Ben W. P. Lew   +21 more
doaj   +4 more sources

Sub-stellar objects with habitable-zone temperatures: A new search for Y dwarfs in WISE [PDF]

open access: diamondEPJ Web of Conferences, 2013
A method is defined for using the maximum sensitivity of WISE to find late T and Y dwarfs. This requires a WISE detection only in the W2-band and uses the statistical properties of the WISE multi-frame measurements and profile fit photometry to reject ...
Day-Jones Avril   +2 more
doaj   +2 more sources

A Tale of Two Molecules: The Underprediction of CO2 and Overprediction of PH3 in Late T and Y Dwarf Atmospheric Models

open access: goldThe Astrophysical Journal
The sensitivity and spectral coverage of JWST are enabling us to test our assumptions of ultracool dwarf atmospheric chemistry, especially with regards to the abundances of phosphine (PH _3 ) and carbon dioxide (CO _2 ).
Samuel A. Beiler   +7 more
doaj   +2 more sources

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