Results 11 to 20 of about 71,830 (288)
Discovery of the Second Y+Y Dwarf Binary System: CWISEP J193518.59-154620.3 [PDF]
We present the discovery of a companion to the Y dwarf, CWISEP J193518.59–154620.3, the second Y-Y dwarf binary detected to date. Y dwarfs are the coldest known free-floating objects (
Matthew De Furio +12 more
doaj +4 more sources
JWST/NIRCam Discovery of the First Y+Y Brown Dwarf Binary: WISE J033605.05–014350.4
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 +6 more sources
Discovery of a new Y dwarf: WISE J030449.03-270508.3 [PDF]
This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record [D. J.
Beletsky, Y. +23 more
core +7 more sources
Y Dwarf Trigonometric Parallaxes from the Spitzer Space Telescope [PDF]
Y dwarfs provide a unique opportunity to study free-floating objects with masses
Beichman, Charles A. +14 more
core +5 more sources
Sub-stellar objects with habitable-zone temperatures: A new search for Y dwarfs in WISE [PDF]
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
Water Clouds in Y Dwarfs and Exoplanets [PDF]
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.
Fortney, Jonathan J. +6 more
core +4 more sources
WISE J163940.83-684738.6: A Y Dwarf identified by Methane Imaging [PDF]
We have used methane imaging techniques to identify the near-infrared counterpart of the bright WISE source WISEJ163940.83-684738.6. The large proper motion of this source (around 3.0arcsec/yr) has moved it, since its original WISE identification, very ...
Cushing, Michael C. +7 more
core +4 more sources
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
JWST 1.5 μm and 4.8 μm Photometry of Y Dwarfs
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 +2 more sources
Exploration of the Near-infrared Colors of Cold Y Dwarfs from the Ground and Space
The James Webb Space Telescope (JWST) has provided critical mid-infrared data for cold brown dwarfs. It has also provided low-resolution near-infrared spectra, and for faint sources these are the first spectra at these wavelengths.
S. K. Leggett +2 more
doaj +3 more sources

