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DYNAMICAL MASS MEASUREMENT OF THE YOUNG SPECTROSCOPIC BINARY V343 NORMAE AaAb RESOLVED WITH THE GEMINI PLANET IMAGER

  • Authors: Eric L. Nielsen, Robert J. De Rosa, Jason Wang, Julien Rameau, Inseok Song, James R. Graham, Bruce Macintosh, Mark Ammons, Vanessa P. Bailey, Travis S. Barman, Joanna Bulger, Jeffrey K. Chilcote, Tara Cotten, Rene Doyon, Gaspard Duchêne, Michael P. Fitzgerald, Katherine B. Follette, Alexandra Z. Greenbaum, Pascale Hibon, Li-Wei Hung, Patrick Ingraham, Paul Kalas, Quinn M. Konopacky, James E. Larkin, Jérôme Maire, Franck Marchis, Mark S. Marley, Christian Marois, Stanimir Metchev, Maxwell A. Millar-Blanchaer, Rebecca Oppenheimer, David W. Palmer, Jenny Patience, Marshall D. Perrin, Lisa A. Poyneer, Laurent Pueyo, Abhijith Rajan, Fredrik T. Rantakyrö, Dmitry Savransky, Adam C. Schneider, Anand Sivaramakrishnan, Remi Soummer, Sandrine Thomas, J. Kent Wallace, Kimberly Ward-Duong, Sloane J. Wiktorowicz, and Schuyler G. Wolff

2016 The Astronomical Journal 152 175.

  • Provider: AAS Journals

Caption: Figure 5.

Comparison of the measured photometry and masses of V343 Nor Aa/Ab (red circles) to the four sets of theoretical models, as well as GJ 3305 A/B (gray diamonds) from Montet et al. (2015), showing good agreement for the expected 20–30 Myr age of the system. For the plotted isochrones, colors corresponds to different models, and linestyles to ages.

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