Dynamical mass measurement of the young spectroscopic binary V343 Normae AaAb resolved with the Gemini Planet Imager
- SETI Institute, Mountain View, CA (United States); Stanford Univ., Stanford, CA (United States)
- Univ. of California, Berkeley, CA (United States)
- Univ. de Montreal, Montreal, QC (Canada)
- Univ. of Georgia, Athens, GA (United States)
- Stanford Univ., Stanford, CA (United States)
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Univ. of Arizona, Tucson, AZ (United States)
- Subaru Telescope, Hilo, HI (United States)
- Univ. of Toronto, Toronto, ON (Canada)
- Univ. of California, Berkeley, CA (United States); Univ. of Grenoble Alpes/CNRS, Grenoble (France)
- Univ. of California, Los Angeles, CA (United States)
- Johns Hopkins Univ., Baltimore, MD (United States)
- European Southern Observatory, Santiago (Chile)
- Large Synoptic Survey Telescope, Tucson, AZ (United States)
- Univ. of California, San Diego, La Jolla, CA (United States)
- SETI Institute, Mountain View, CA (United States)
- NASA Ames Research Center (ARC), Moffett Field, CA (United States)
- National Research Council of Canada Herzberg, Victoria, BC (Canada); Univ. of Victoria, Victoria, BC (Canada)
- The Univ. of Western Ontario, London, ON (Canada); Stony Brook Univ., Stony Brook, NY (United States)
- American Museum of Natural History, New York, NY (United States)
- Arizona State Univ., Tempe, AZ (United States)
- Space Telescope Science Institute, Baltimore, MD (United States)
- Gemini Observatory, La Serena (Chile)
- Cornell Univ., Ithaca, NY (United States)
- Univ. of Toledo, Toledo, OH (United States)
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
- The Aerospace Corp., El Segundo, CA (United States)
Here, 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 $${M}_{\mathrm{Aa}}=1.10\pm 0.10\,{M}_{\odot }$$ and $${M}_{\mathrm{Ab}}=0.290\pm 0.018\,{M}_{\odot }$$. 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.
- Research Organization:
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Sponsoring Organization:
- USDOE
- Grant/Contract Number:
- AC52-07NA27344
- OSTI ID:
- 1352126
- Report Number(s):
- LLNL-JRNL-717862; TRN: US1701222
- Journal Information:
- The Astronomical Journal (Online), Vol. 152, Issue 6; ISSN 1538-3881
- Publisher:
- IOP PublishingCopyright Statement
- Country of Publication:
- United States
- Language:
- English
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