TY - JOUR
T1 - DYNAMICAL MASS MEASUREMENT of the YOUNG SPECTROSCOPIC BINARY V343 NORMAE AaAb RESOLVED with the GEMINI PLANET IMAGER
AU - Nielsen, Eric L.
AU - Rosa, Robert J.De
AU - Wang, Jason
AU - Rameau, Julien
AU - Song, Inseok
AU - Graham, James R.
AU - Macintosh, Bruce
AU - Ammons, Mark
AU - Bailey, Vanessa P.
AU - Barman, Travis S.
AU - Bulger, Joanna
AU - Chilcote, Jeffrey K.
AU - Cotten, Tara
AU - Doyon, Rene
AU - Duchene, Gaspard
AU - Fitzgerald, Michael P.
AU - Follette, Katherine B.
AU - Greenbaum, Alexandra Z.
AU - Hibon, Pascale
AU - Hung, Li Wei
AU - Ingraham, Patrick
AU - Kalas, Paul
AU - Konopacky, Quinn M.
AU - Larkin, James E.
AU - Maire, Jérôme
AU - Marchis, Franck
AU - Marley, Mark S.
AU - Marois, Christian
AU - Metchev, Stanimir
AU - Millar-Blanchaer, Maxwell A.
AU - Oppenheimer, Rebecca
AU - Palmer, David W.
AU - Patience, Jenny
AU - Perrin, Marshall D.
AU - Poyneer, Lisa A.
AU - Pueyo, Laurent
AU - Rajan, Abhijith
AU - Rantakyrö, Fredrik T.
AU - Savransky, Dmitry
AU - Schneider, Adam C.
AU - Sivaramakrishnan, Anand
AU - Soummer, Remi
AU - Thomas, Sandrine
AU - Wallace, J. Kent
AU - Ward-Duong, Kimberly
AU - Wiktorowicz, Sloane J.
AU - Wolff, Schuyler G.
N1 - Publisher Copyright:
© 2016. The American Astronomical Society. All rights reserved.
PY - 2016/12
Y1 - 2016/12
N2 - We present new spatially resolved astrometry and photometry from the Gemini Planet Imager of the inner binary of the young multiple star system V343 Normae, which is a member of the β Pictoris (β Pic) moving group. V343 Normae comprises a K0 and mid-M star in a ∼4.5 year orbit (AaAb) and a wide 10″ M5 companion (B). By combining these data with archival astrometry and radial velocities we fit the orbit and measure individual masses for both components of MAa = 1.10 ± 0.10 M⊙ and MAb = 0.290 ± 0.018 M⊙. Comparing to theoretical isochrones, we find good agreement for the measured masses and JHK band magnitudes of the two components consistent with the age of the β Pic moving group. We derive a model-dependent age for the β Pic moving group of 26 ±3 Myr by combining our results for V343 Normae with literature measurements for GJ 3305, which is another group member with resolved binary components and dynamical masses.
AB - We present new spatially resolved astrometry and photometry from the Gemini Planet Imager of the inner binary of the young multiple star system V343 Normae, which is a member of the β Pictoris (β Pic) moving group. V343 Normae comprises a K0 and mid-M star in a ∼4.5 year orbit (AaAb) and a wide 10″ M5 companion (B). By combining these data with archival astrometry and radial velocities we fit the orbit and measure individual masses for both components of MAa = 1.10 ± 0.10 M⊙ and MAb = 0.290 ± 0.018 M⊙. Comparing to theoretical isochrones, we find good agreement for the measured masses and JHK band magnitudes of the two components consistent with the age of the β Pic moving group. We derive a model-dependent age for the β Pic moving group of 26 ±3 Myr by combining our results for V343 Normae with literature measurements for GJ 3305, which is another group member with resolved binary components and dynamical masses.
KW - planets and satellites: detection
KW - stars: individual (V343 Nor)
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U2 - 10.3847/0004-6256/152/6/175
DO - 10.3847/0004-6256/152/6/175
M3 - Article
AN - SCOPUS:85009115867
SN - 0004-6256
VL - 152
JO - Astronomical Journal
JF - Astronomical Journal
IS - 6
M1 - 175
ER -