Results 111 to 120 of about 10,855,464 (193)
A Survey of Model Fits to Brown Dwarf Spectra Through the L–T Sequence
We fit archival near-IR spectra of ∼300 brown dwarfs with atmosphere models from the Sonora and Phoenix groups. Using the parameters of the best-fit models as estimates for the physical properties of the brown dwarfs in our sample, we have performed a ...
Savanah K. Turner +3 more
doaj +1 more source
The Kinematic Age of the Coolest T Dwarfs
Article version of a poster paper at Cool Stars 17, Barcelona, June ...
Smith, Leigh +7 more
openaire +2 more sources
Discovery of a t dwarf plus white dwarf binary system
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Day-Jones, A. C. +13 more
openaire +5 more sources
We present the discovery of 11 new T dwarfs, found during the course of a photometric survey for mid-to-late T dwarfs in the 2MASS Point Source Catalog and from a proper-motion-selected sample of ultracool dwarfs in the 2MASS Working Database.
J. Davy Kirkpatrick +2 more
core +1 more source
Di scovery of a T dwarf + white dwarf binary system
We present the discovery of the first T dwarf + white dwarf binary system LSPM 1459+0857AB, confirmed through common proper motion and spectroscopy. The white dwarf is a high proper motion object from the LSPM catalogue that we confirm spectroscopically ...
Day-Jones, A.C. +2 more
openaire +4 more sources
On the Orbit of the Binary Brown Dwarf Companion GL229 Ba and Bb
The companion GL229B was recently resolved by Xuan et al. as a tight binary of two brown dwarfs (Ba and Bb) through VLTI-GRAVITY interferometry and Very Large Telescope-CRIRES+ radial velocity (RV) measurements.
William Thompson +23 more
doaj +1 more source
Cool versus ultracool white dwarfs [PDF]
A preliminary BVRIJHK analysis of the white dwarfs SSSPM J2231-7514 and SSSPM J2231-7515 is presented. Although both stars were reported to have T eff < 4000 K, the analysis here indicates T eff ≈ 4250 K for both SSSPM J2231-7514 and SSSPM J2231-7515 ...
Farihi, J
core
We present the most precise constraints to date for the mass and age distributions of single ultracool dwarfs in the solar neighborhood, based on an updated volume-limited sample of 504 L, T, and Y dwarfs within 25 pc.
William M. J. Best +4 more
doaj +1 more source
Constraints on Remnant Planetary Systems as a Function of Main-sequence Mass with HST/COS
As the descendants of stars with masses less than 8 M _⊙ on the main sequence, white dwarfs provide a unique way to constrain planetary occurrence around intermediate-mass stars (spectral types BAF) that are otherwise difficult to measure with radial ...
Lou Baya Ould Rouis +10 more
doaj +1 more source
Disequilibrium chemistry due to vertical mixing in the atmospheres of many brown dwarfs and giant exoplanets is well established. Atmosphere models for these objects typically parameterize mixing with the highly uncertain K _zz diffusion parameter.
Sagnick Mukherjee +9 more
doaj +1 more source

