Results 51 to 60 of about 22,040,331 (192)
The GALAH Survey : Lithium-strong KM dwarfs [PDF]
Identifying and characterizing young stars in the Solar neighbourhood is essential to find and describe planets in the early stages of their evolution. This work seeks to identify nearby young stars showing a lithium 6708 Å absorption line in the GALAH ...
Martell, S., +35 more
core +1 more source
Infrared Excesses around Bright White Dwarfs from Gaia and unWISE. II [PDF]
Infrared excesses around white dwarf stars indicate the presence of various astrophysical objects of interest, including companions and debris disks. In this second paper of a series, we present follow-up observations of infrared excess candidates from ...
Kleinman, Scot J. +23 more
core +1 more source
Dynamics of Y dwarf atmospheres
Context . The global circulation regime of the coolest class of brown dwarfs, known as the Y dwarfs, remains largely unexplored. Aims .
C. Akın +3 more
openaire +2 more sources
Keck NIRES Spectral Standards for L, T, and Y Dwarfs
Abstract We present medium-resolution (λ/Δλ = 2700), near-infrared spectral standards for field L0–L2, L4, and L7–Y0 dwarfs obtained with the Near-Infrared Echellette Spectrometer on the Keck II 10 m telescope. These standards allow for detailed spectral comparative analysis of cold brown dwarfs discovered through ongoing ground-based ...
Christopher A. Theissen +16 more
openaire +2 more sources
CFBDS J005910.90-011401.3: reaching the T-Y brown dwarf transition? [PDF]
12 pages, Submitted to A& ...
Delorme, Philippe +11 more
openaire +6 more sources
THE FIRST DETECTION OF PHOTOMETRIC VARIABILITY IN A Y DWARF: WISE J140518.39+553421.3 [PDF]
ABSTRACT We present the first detection of the photometric variability in a spectroscopically confirmed Y dwarf. The Infrared Array Camera on board the Spitzer Space Telescope was used to obtain time series photometry of WISE J140518.39+553421.3 at 3.6 and 4.5
Michael C. Cushing +10 more
openaire +4 more sources
The discovery of y dwarfs using data from the wide-field infrared survey explorer (WISE) [PDF]
We present the discovery of seven ultracool brown dwarfs identified with the Wide-field Infrared Survey Explorer (WISE). Near-infrared spectroscopy reveals deep absorption bands of H[subscript 2]O and CH[subscript 4] that indicate all seven of the brown ...
Gelino, Christopher R. +31 more
core +1 more source
CARMENES input catalogue of M dwarfs [PDF]
Aims. Our goals are to characterise the kinematic properties and to identify young and old stars among the M dwarfs of the CARMENES input catalogue. Methods.
Jeffers, S. +54 more
core +1 more source
The Y dwarf CWISEP J193518.59-154620.3 (WISE 1935 or W1935) exhibits a thermal inversion in its radiative atmosphere, producing methane emission features in its JWST spectrum, but the physical mechanism responsible for this inversion remains unknown ...
Kayla J. Smith +3 more
doaj +1 more source
Atmospheric Retrieval Of Cool Y Dwarfs
Brown dwarfs' near-infrared spectra contain a wealth of information which can reveal the physical and chemical processes that occur in their atmospheres. Using a recently developed atmospheric retrieval model, we are able to constrain various molecular abundances, along with photometric radius, gravity, cloud optical depths, and temperature profiles ...
Zalesky, Joseph +2 more
openaire +2 more sources

