NLTT 41135: A FIELD M DWARF + BROWN DWARF ECLIPSING BINARY IN A TRIPLE SYSTEM, DISCOVERED BY THE MEARTH OBSERVATORY
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Author(s)
Irwin, Jonathan
Buchhave, Lars
Berta, Zachory K.
Charbonneau, David
Latham, David W.
Burke, Christopher J.
Esquerdo, Gilbert A.
Everett, Mark E.
Holman, Matthew J.
Nutzman, Philip
Date Issued
July 2010
Journal
Astrophysical Journal
Publisher
American Astronomical Society/IOP Publishing
Citation
Irwin, Jonathan et al. “NLTT 41135: A FIELD M DWARF + BROWN DWARF ECLIPSING BINARY IN A TRIPLE SYSTEM, DISCOVERED BY THE MEARTH OBSERVATORY.” The Astrophysical Journal 718, 2 (July 2010): 1353–1366 © 2010 The American Astronomical Society
Version
Final published version
Abstract
We report the discovery of an eclipsing companion to NLTT 41135, a nearby M5 dwarf that was already known to have a wider, slightly more massive common proper motion companion, NLTT 41136, at 2″.4 separation. Analysis of combined-light and RV curves of the system indicates that NLTT 41135B is a (31-34) ± 3M Jup brown dwarf (where the range depends on the unknown metallicity of the host star) on a circular orbit. The visual M dwarf pair appears to be physically bound, so the system forms a hierarchical triple, with masses approximately in the ratio 8:6:1. The eclipses are grazing, preventing an unambiguous measurement of the secondary radius, but follow-up observations of the secondary eclipse (e.g., with the James Webb Space Telescope) could permit measurements of the surface brightness ratio between the two objects, and thus place constraints on models of brown dwarfs.
MIT Department
Massachusetts Institute of Technology. Department of Physics
MIT Kavli Institute for Astrophysics and Space Research
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DOI of Published Version
https://doi.org/10.1088/0004-637X/718/2/1353
