Abstract
In our effort to complete the census of low-mass stars and brown dwarfs in the immediate Solar Neighborhood, we present spectra, photometry, proper motions, and distance estimates for forty-two low-mass star and brown dwarf candidates discovered by the Wide-field Infrared Survey Explorer (WISE). We also present additional follow-up information on twelve candidates selected using WISE data but previously published elsewhere. The new discoveries include fifteen M dwarfs, seventeen L dwarfs, five T dwarfs, and five objects of other type. Among these discoveries is a newly identified "unusually red L dwarf" (WISE J223527.07+451140.9), four peculiar L dwarfs whose spectra are most readily explained as unresolved L+T binary systems, and a T9 dwarf (WISE J124309.61+844547.8). We also show that the recently discovered red L dwarf WISEP J004701.06+680352.1 (Gizis et al. 2012) may be a low-gravity object and hence young and potentially low mass (< 25 MJup).
Cite
CITATION STYLE
Thompson, M. A., Kirkpatrick, J. D., Mace, G. N., Cushing, M. C., Gelino, C. R., Griffith, R. L., … Bloom, J. S. (2013). Nearby M, L, and T Dwarfs Discovered by the Wide-field Infrared Survey Explorer ( WISE ). Publications of the Astronomical Society of the Pacific, 125(929), 809–837. https://doi.org/10.1086/671426
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.