Parallaxes and Infrared Photometry of three Y0 dwarfs
arXiv:1703.10341 · doi:10.1093/mnras/stx723
Abstract
We have followed up the three Y0 dwarfs WISEPA J041022.71+150248.5, WISEPA J173835.53+273258.9 and WISEPC J205628.90+145953.3 using the UKIRT/WFCAM telescope/instruments. We find parallaxes that are more consistent and accurate than previously published values. We estimate absolute magnitudes in photometric pass-bands from to and find them to be consistent between the three Y0 dwarfs indicating the inherent cosmic absolute magnitude spread of these objects is small. We examine the MKO magnitudes over the four year time line and find small but significant monotonic variations. Finally we estimate physical parameters from a comparison of spectra and parallax to equilibrium and non-equilibrium models finding values consistent with solar metallicity, an effective temperature of 450-475\,K and log~g of 4.0-4.5.
12 Pages, 10 figures, Accepted by MNRAS
References in corpus (12)
- The Evolution of L and T Dwarfs in Color-Magnitude Diagrams
- The UKIRT Wide Field Camera ZYJHK Photometric System: Calibration from 2MASS
- Fingering convection and cloudless models for cool brown dwarf atmospheres
- The UKIRT Infrared Deep Sky Survey Early Data Release
- Water Clouds in Y Dwarfs and Exoplanets
- Hubble Space Telescope Spectroscopy of Brown Dwarfs Discovered with the Wide-field Infrared Survey Explorer
- : Pressure-dependent Changes In Light Curve Phase In Brown Dwarfs From Simultaneous and Observations
- Near-infrared photometry of Y dwarfs: low ammonia abundance and the onset of water clouds
- The Luminosities of the Coldest Brown Dwarfs
- Saturn's Great Storm of 2010-2011: Evidence for ammonia and water ices from analysis of VIMS spectra
- Observed Variability at 1um and 4um in the Y0 Brown Dwarf WISEP J173835.52+273258.9
- Photometric Monitoring of the Coldest Known Brown Dwarf with the Spitzer Space Telescope
Cited by in corpus (7)
- Preliminary Trigonometric Parallaxes of 184 Late-T and Y Dwarfs and an Analysis of the Field Substellar Mass Function into the "Planetary" Mass Regime
- The Hawaii Infrared Parallax Program. IV. A Comprehensive Parallax Survey of L0-T8 dwarfs with UKIRT
- A Uniform Retrieval Analysis of Ultracool Dwarfs. III. Properties of Y-Dwarfs
- A 3D view of the Hyades stellar and sub-stellar population
- Y dwarf Trigonometric Parallaxes from the Spitzer Space Telescope
- Parallaxes of southern extremely cool objects III: 118 L \& T dwarfs
- Parallaxes of Cool Objects with WISE: Filling in for Gaia