Iras-allsky

Discovery of the benchmark metal-poor T8 dwarf BD +01° 2920B

May 2012 • 2012MNRAS.422.1922P

Authors • Pinfield, D. J. • Burningham, B. • Lodieu, N. • Leggett, S. K. • Tinney, C. G. • van Spaandonk, L. • Marocco, F. • Smart, R. • Gomes, J. • Smith, L. • Lucas, P. W. • Day-Jones, A. C. • Murray, D. N. • Katsiyannis, A. C. • Catalan, S. • Cardoso, C. • Clarke, J. R. A. • Folkes, S. • Gálvez-Ortiz, M. C. • Homeier, D. • Jenkins, J. S. • Jones, H. R. A. • Zhang, Z. H.

Abstract • We have searched the Wide-field Infrared Survey Explorer first data release for widely separated (≤10 000 au) late T dwarf companions to Hipparcos and Gliese stars. We have discovered a new binary system containing a K-band suppressed T8p dwarf WISEP J142320.86+011638.1 and the mildly metal poor ([Fe/H] =-0.38 ± 0.06) primary BD +01° 2920 (HIP 70319), a G1 dwarf at a distance of 17.2 pc. This new benchmark has Teff= 680 ± 55 K and a mass of 20-50MJup. Its spectral properties are well modelled except for known discrepancies in the Y and K bands. Based on the well-determined metallicity of its companion, the properties of BD +01° 2920B imply that the currently known T dwarfs are dominated by young low-mass objects. We also present an accurate proper motion for the T8.5 dwarf WISEP J075003.84+272544.8.

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Federico Marocco

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