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 latetype 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 M⊙1). This object may thus be extending the population parameter space of the known Y0 dwarfs.
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CITATION STYLE
Pinfield, D. J., Gromadzki, M., Leggett, S. K., Gomes, J., Lodieu, N., Kurtev, R., … Zhang, Z. (2014). Discovery of a new Y dwarf: WISE J030449.03-270508.3. Monthly Notices of the Royal Astronomical Society, 444(2), 1931–1939. https://doi.org/10.1093/mnras/stu1540
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