Discovery of a Substellar Companion to the Nearby Debris Disk Host HR 2562

@article{Konopacky2016DiscoveryOA,
  title={Discovery of a Substellar Companion to the Nearby Debris Disk Host HR 2562},
  author={Quinn M. Konopacky and Julien Rameau and Gaspard Duch{\^e}ne and Joseph C. Filippazzo and Paige A. Giorla Godfrey and Christian Marois and Eric L. Nielsen and Laurent Pueyo and Roman R. Rafikov and Emily L. Rice and Jason J. Wang and S. Mark Ammons and Vanessa P. Bailey and Travis S. Barman and Joanna Bulger and Sebastian Bruzzone and Jeffrey K. Chilcote and Tara Cotten and Rebekah I. Dawson and Robert J. De Rosa and Ren{\'e} Doyon and Thomas M. Esposito and Michael P. Fitzgerald and Katherine B. Follette and Stephen J. Goodsell and James R. Graham and Alexandra Z. Greenbaum and Pascale Hibon and Li-Wei Hung and Patrick Ingraham and Paul Kalas and David Lafreni{\`e}re and James E. Larkin and Bruce A. Macintosh and J'erome Maire and Franck Marchis and Mark S. Marley and Brenda C. Matthews and Stanimir Metchev and Maxwell A. Millar-Blanchaer and Rebecca Oppenheimer and David Palmer and Jennifer Lynn Patience and Marshall D. Perrin and Lisa Ann Poyneer and Abhijith Rajan and Fredrik T. Rantakyro and Dmitry Savransky and Adam C. Schneider and Anand Sivaramakrishnan and Inseok Song and R{\'e}mi Soummer and Sandrine J. Thomas and James K. Wallace and Kimberley Ward-Duong and Sloane J. Wiktorowicz and Schuyler G. Wolff},
  journal={arXiv: Earth and Planetary Astrophysics},
  year={2016}
}
We present the discovery of a brown dwarf companion to the debris disk host star HR 2562. This object, discovered with the Gemini Planet Imager (GPI), has a projected separation of 20.3$\pm$0.3 au (0.618$\pm$0.004") from the star. With the high astrometric precision afforded by GPI, we have confirmed common proper motion of HR 2562B with the star with only a month time baseline between observations to more than $5\sigma$. Spectral data in $J$, $H$, and $K$ bands show morphological similarity to… Expand
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