Exploring the substellar temperature regime down to ~550K
Ben Burningham, D. J. Pinfield, S. K. Leggett, M. Tamura, P. W. Lucas,, D. Homeier, A. Day-Jones, H. R. A. Jones, J.R.A. Clarke, M. Ishii, M., Kuzuhara, N. Lodieu, M. R. Zapatero Osorio, B.P. Venemans, D.J. Mortlock, D., Barrado y Navascues, E. L. Martin, A. Magazzu

TL;DR
This paper reports the discovery of three very late T dwarfs, extending the substellar temperature regime down to approximately 550K, and provides detailed photometric, spectroscopic, and modeling analysis of these ultra-cool objects.
Contribution
It introduces new late T dwarf discoveries, extends spectral classification schemes to T9, and estimates their physical properties, including the coolest temperature measurements for such objects.
Findings
ULAS1335 has an estimated temperature below 600K.
ULAS1335 is the reddest T dwarf observed in near to mid-infrared colors.
ULAS1335's temperature is approximately 550-600K.
Abstract
We report the discovery of three very late T dwarfs in the UKIRT Infrared Deep Sky Survey (UKIDSS) Third Data Release: ULAS J101721.40+011817.9 (ULAS1017), ULAS J123828.51+095351.3 (ULAS1238) and ULAS J133553.45+113005.2 (ULAS1335).We detail optical and near-infrared photometry for all three sources, and mid-infrared photometry for ULAS1335. We use near-infrared spectra of each source to assign spectral types T8p (ULAS1017), T8.5 (ULAS1228) and T9 (ULAS1335) to these objects. We estimate that ULAS1017 has 750 < Teff < 850K, and 5.0 < log g < 5.5, assuming solar metallicity, an age of 1.6-15 Gyr, a mass of 33-70 MJ and lies at a distance of 31-54 pc. We extend the unified scheme of Burgasser et al. (2006) to the type T9 and suggest the inclusion of the WJ index to replace the now saturated J-band indices. ULAS1335 is the same spectral type as ULAS J003402.77-005206.7 and CFBDS…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astrophysics and Star Formation Studies
