Abstract
The Wide-field Infrared Survey Explorer has revealed a T8.5 brown dwarf (WISE J111838.70+312537.9) that exhibits common proper motion with a solar-neighborhood (8 pc) quadruple star system - ξ Ursae Majoris. The angular separation is 8.′5, and the projected physical separation is ≈4000 AU. The sub-solar metallicity and low chromospheric activity of ξ UMa A argue that the system has an age of at least 2 Gyr. The infrared luminosity and color of the brown dwarf suggests the mass of this companion ranges between 14 and 38 MJ for system ages of 2 and 8 Gyr, respectively.
Original language | English (US) |
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Article number | 84 |
Journal | Astronomical Journal |
Volume | 145 |
Issue number | 3 |
DOIs | |
State | Published - Mar 2013 |
Externally published | Yes |
Keywords
- brown dwarfs
- infrared: stars
- solar neighborhood
- stars: late-type
- stars: low-mass
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science