A study of the diverse T dwarf population revealed by wise

Gregory N. Mace, J. Davy Kirkpatrick, Michael C. Cushing, Christopher R. Gelino, Roger L. Griffith, Michael F. Skrutskie, Kenneth A. Marsh, Edward L. Wright, Peter R. Eisenhardt, Ian S. McLean, Maggie A. Thompson, Katholeen Mix, Vanessa Bailey, Charles A. Beichman, Joshua S. Bloom, Adam J. Burgasser, Jonathan J. Fortney, Philip M. Hinz, Russell P. Knox, Patrick J. LowranceMark S. Marley, Caroline V. Morley, Timothy J. Rodigas, Didier Saumon, Scott S. Sheppard, Nathan D. Stock

Research output: Contribution to journalArticle

65 Scopus citations

Abstract

We report the discovery of 87 new T dwarfs uncovered with the Wide-field Infrared Survey Explorer (WISE) and 3 brown dwarfs with extremely red near-infrared colors that exhibit characteristics of both L and T dwarfs. Two of the new T dwarfs are likely binaries with L7 ± 1 primaries and mid-type T secondaries. In addition, our follow-up program has confirmed 10 previously identified T dwarfs and 4 photometrically selected L and T dwarf candidates in the literature. This sample, along with the previous WISE discoveries, triples the number of known brown dwarfs with spectral types later than T5. Using the WISE All-Sky Source Catalog we present updated color-color and color-type diagrams for all the WISE-discovered T and Y dwarfs. Near-infrared spectra of the new discoveries are presented along with spectral classifications. To accommodate later T dwarfs we have modified the integrated flux method of determining spectral indices to instead use the median flux. Furthermore, a newly defined J-narrow index differentiates the early-type Y dwarfs from late-type T dwarfs based on the J-band continuum slope. The K/J indices for this expanded sample show that 32% of late-type T dwarfs have suppressed K-band flux and are blue relative to the spectral standards, while only 11% are redder than the standards. Comparison of the Y/J and K/J index to models suggests diverse atmospheric conditions and supports the possible re-emergence of clouds after the L/T transition. We also discuss peculiar brown dwarfs and candidates that were found not to be substellar, including two young stellar objects and two active galactic nuclei. The substantial increase in the number of known late-type T dwarfs provides a population that will be used to test models of cold atmospheres and star formation. The coolest WISE-discovered brown dwarfs are the closest of their type and will remain the only sample of their kind for many years to come.

Original languageEnglish (US)
Article number6
JournalAstrophysical Journal, Supplement Series
Volume205
Issue number1
DOIs
StatePublished - Mar 1 2013

Keywords

  • binaries: general
  • brown dwarfs
  • galaxies: active
  • infrared: stars
  • stars: low-mass

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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    Mace, G. N., Davy Kirkpatrick, J., Cushing, M. C., Gelino, C. R., Griffith, R. L., Skrutskie, M. F., Marsh, K. A., Wright, E. L., Eisenhardt, P. R., McLean, I. S., Thompson, M. A., Mix, K., Bailey, V., Beichman, C. A., Bloom, J. S., Burgasser, A. J., Fortney, J. J., Hinz, P. M., Knox, R. P., ... Stock, N. D. (2013). A study of the diverse T dwarf population revealed by wise. Astrophysical Journal, Supplement Series, 205(1), [6]. https://doi.org/10.1088/0067-0049/205/1/6