The First Ultra-cool Brown Dwarf Discovered by the Wide-field Infrared Survey Explorer
Abstract
We report the discovery of the first new ultra-cool brown dwarf (BDs) found with the Wide-field Infrared Survey Explorer (WISE). The object's preliminary designation is WISEPC J045853.90+643451.9. Follow-up spectroscopy with the LUCIFER instrument on the Large Binocular Telescope indicates that it is a very late-type T dwarf with a spectral type approximately equal to T9. Fits to an IRTF/SpeX 0.8-2.5 μm spectrum to the model atmospheres of Marley and Saumon indicate an effective temperature of approximately 600 K as well as the presence of vertical mixing in its atmosphere. The new BD is easily detected by WISE, with a signal-to-noise ratio of ~36 at 4.6 μm. Current estimates place it at a distance of 6-10 pc. This object represents the first in what will likely be hundreds of nearby BDs found by WISE that will be suitable for follow-up observations, including those with the James Webb Space Telescope. One of the two primary scientific goals of the WISE mission is to find the coolest, closest stars to our Sun; the discovery of this new BD proves that WISE is capable of fulfilling this objective.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- January 2011
- DOI:
- 10.1088/0004-637X/726/1/30
- arXiv:
- arXiv:1011.2279
- Bibcode:
- 2011ApJ...726...30M
- Keywords:
-
- brown dwarfs;
- infrared: stars;
- solar neighborhood;
- stars: late-type;
- stars: low-mass;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- 23 pages, 2010 ApJ accepted