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Title: HII 2407: AN ECLIPSING BINARY REVEALED BY K2 OBSERVATIONS OF THE PLEIADES

Journal Article · · Astrophysical Journal
; ; ;  [1]; ;  [2];  [3]; ;  [4]; ; ;  [5];  [6];  [7]; ;  [8]; ;  [9];  [10]
  1. Department of Astronomy, California Institute of Technology, Pasadena, CA 91125 (United States)
  2. Spitzer Science Center, California Institute of Technology, Pasadena, CA 91125 (United States)
  3. NASA Ames Research Center, Mountain View, CA 94035 (United States)
  4. Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235 (United States)
  5. Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH (United Kingdom)
  6. SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS (United Kingdom)
  7. Centro de Astrobiología, INTA-CSIC, Dpto. Astrofísica, ESAC Campus, P.O. Box 78, E-28691 Villanueva de la Cañada, Madrid (Spain)
  8. Department of Astronomy, University of California, Berkeley, CA 94720 (United States)
  9. Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Chapel Hill, NC 27599-3255 (United States)
  10. Institute for Astronomy, University of Hawai‘i at Mānoa, Hilo, HI 96720-2700 (United States)

The star HII 2407 is a member of the relatively young Pleiades star cluster and was previously discovered to be a single-lined spectroscopic binary. It is newly identified here within Kepler/K2 photometric time series data as an eclipsing binary system. Mutual fitting of the radial velocity and photometric data leads to an orbital solution and constraints on fundamental stellar parameters. While the primary has arrived on the main sequence, the secondary is still pre-main sequence and we compare our results for the M/M{sub ⊙} and R/R{sub ⊙} values with stellar evolutionary models. We also demonstrate that the system is likely to be tidally synchronized. Follow-up infrared spectroscopy is likely to reveal the lines of the secondary, allowing for dynamically measured masses and elevating the system to benchmark eclipsing binary status.

OSTI ID:
22521892
Journal Information:
Astrophysical Journal, Vol. 814, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English