Discovery of a new Y dwarf: WISE J030449.03-270508.3

Pinfield, D.J., Gromadzki, M., Leggett, S.K., Gomes, J., Lodieu, N., Kurtev, R., Day-Jones, A. C., Ruiz, M. T., Cook, N. J., Morley, C.V., Marley, M. S., Marocco, F., Smart, R.L., Jones, H.R.A., Lucas, P.W., Beletsky, Y., Ivanov, V. D., Burningham, B., Jenkins, J. S., Cardoso, C., Frith, J., Clarke, J. R. A., Gálvez-Ortiz, M. C. and Zhang, Z. (2014) Discovery of a new Y dwarf: WISE J030449.03-270508.3. pp. 1931-1939. ISSN 0035-8711
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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.

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