Abstract
The discovery and subsequent detailed study of T dwarfs have provided many surprises and pushed the physics and modelling of cool atmospheres in unpredicted directions. Distance is a critical parameter for studies of these objects to determine intrinsic luminosities, test binarity and measure their motion in the Galaxy. We describe a new observational programme to determine distances across the full range of T-dwarf subtypes using the New Technology Telescope (NTT)/SOFI telescope/instrument combination. We present preliminary results for ten objects, five of which represent new distances.
Original language | English |
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Pages (from-to) | 2054-2063 |
Number of pages | 10 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 433 |
Issue number | 3 |
DOIs | |
Publication status | Published - Aug 2013 |
Keywords
- methods: data analysis
- astrometry
- parallaxes
- proper motions
- brown dwarfs
- T-DWARF SEARCH
- ALL-SKY SURVEY
- ULTRACOOL BROWN DWARFS
- LARGE-AREA SURVEY
- L/T TRANSITION
- SPECTRAL CLASSIFICATION
- PROPER MOTIONS
- 2MASS
- DISCOVERY
- BINARY