Blue not brown: UKIDSS T dwarfs with suppressed K-band flux
D. N. Murray, B. Burningham, H. R. A Jones, D. J. Pinfield, P. W., Lucas, S. K. Leggett, C. G. Tinney, A. C. Day-Jones, D. J. Weights, N., Lodieu, J. A. Perez Prieto, E. Nickson, Z. H. Zhang, J. R. A. Clarke, J. S., Jenkins, M. Tamura

TL;DR
This study identifies and characterizes a group of T dwarfs with blue near-infrared colours, including potential halo members and a metal-poor benchmark, using proper motions, distances, and velocities.
Contribution
First identification of halo T-dwarf candidates and a metal-poor benchmark T dwarf using blue near-infrared colours and kinematic analysis.
Findings
Two potential halo T-dwarf candidates with high velocities.
Discovery of a metal-poor T dwarf benchmark, Hip 73786B.
Blue colours linked to high gravity or low metallicity.
Abstract
We have used blue near-infrared colours to select a group of 12 spectroscopically-confirmed UKIDSS T dwarfs later than T4. From amongst these we identify the first two kinematic halo T-dwarf candidates. Blue near-infrared colours have been attributed to collisionally-induced hydrogen absorption, which is enhanced by either high surface gravity or low metallicity. Proper motions are measured and distances estimated, allowing the determination of tangential velocities. U and V components are estimated for our objects by assuming radial velocity = 0 km/s. From this, ULAS J0926+0835 is found to have U=62 km/s and V=-140km/s and ULAS J1319+1209 is found to have U=192 km/s and V=-92 km/s. These values are consistent with potential halo membership. However, these are not the bluest objects in our selection. The bluest is ULAS J1233+1219, with J-K=-1.16 +/- 0.07, and surprisingly this object is…
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