Abstract
We present a new Y dwarf, WISE J030449.03−270508.3, confirmed from a candidate sample designed to pick out low-temperature objects from the Wide-field Infrared Survey Explorer (WISE) data base. The new object is typed Y0pec following a visual comparison with spectral standards, and lies at a likely distance of 10–17 pc. Its tangential velocity suggests thin disc membership, but it shows some spectral characteristics that suggest that it may be metal poor and/or older than previously identified Y0 dwarfs. Based on trends seen for warmer late-type T dwarfs, the Y-band flux peak morphology is indicative of sub-solar metallicity, and the enhanced red wing of the J-band flux peak offers evidence for high gravity and/or low metallicity (with associated model trends suggesting an age closer to ∼10 Gyr and mass in the range 0.02–0.03 Mȯ). This object may thus be extending the population parameter space of the known Y0 dwarfs.
Original language | English |
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Article number | stu1540 |
Pages (from-to) | 1931-1939 |
Number of pages | 9 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 444 |
Issue number | 2 |
Early online date | 4 Sept 2014 |
DOIs | |
Publication status | Published - 21 Oct 2014 |
Keywords
- Brown dwarfs
- Stars: Low-mass
- Surveys