A T8.5 BROWN DWARF MEMBER OF THE {xi} URSAE MAJORIS SYSTEM
Journal Article
·
· Astronomical Journal (New York, N.Y. Online)
- UCLA Astronomy, P.O. Box 951547, Los Angeles, CA 90095-1547 (United States)
- Department of Astronomy, University of Virginia, Charlottesville, VA 22904 (United States)
- Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States)
- School of Physics and Astronomy, Cardiff University, Cardiff CF243AA (United Kingdom)
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109-8001 (United States)
- National Radio Astronomy Observatory, Charlottesville, VA 22903 (United States)
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-{xi} Ursae Majoris. The angular separation is 8.'5, and the projected physical separation is Almost-Equal-To 4000 AU. The sub-solar metallicity and low chromospheric activity of {xi} 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 M{sub J} for system ages of 2 and 8 Gyr, respectively.
- OSTI ID:
- 22130859
- Journal Information:
- Astronomical Journal (New York, N.Y. Online), Vol. 145, Issue 3; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1538-3881
- Country of Publication:
- United States
- Language:
- English
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