Discovery of a 0.15" Binary Brown Dwarf 2MASSJ 1426316+155701 With Gemini/Hokupa'a Adaptive Optics
arXiv:astro-ph/0110669 · doi:10.1086/337916
Abstract
Use of the highly sensitive Hokupa'a curvature wavefront sensor has allowed for the first time direct adaptive optics (AO) guiding on brown dwarfs and VLM stars (SpT=M7-L2). An initial survey of 9 such objects discovered one 0.15" binary (2MASSJ 1426316+155701). The companion is about half as bright as the primary (Delta K = 0.61+/-0.05. These spectral types also match the observed H-K colors of each star. Based the previously observed low space motion and activity we assign an age of . Utilizing this age range and the latest DUSTY models of the Lyon group we assign a photometric distance of and masses of and . We therefore estimate a system separation of and a period of respectively. Hence, 2M1426 is among the smallest separation brown dwarf binaries resolved to date.
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