The Astronomical Journal (Jan 2023)

HIP 33609 b: An Eccentric Brown Dwarf Transiting a V = 7.3 Rapidly Rotating B Star

  • Noah Vowell,
  • Joseph E. Rodriguez,
  • Samuel N. Quinn,
  • George Zhou,
  • Andrew Vanderburg,
  • Andrew W. Mann,
  • Matthew J. Hooton,
  • Keivan G. Stassun,
  • Saburo Howard,
  • Allyson Bieryla,
  • David W. Latham,
  • Steve B. Howell,
  • Tristan Guillot,
  • Carl Ziegler,
  • Karen A. Collins,
  • Theron W. Carmichael,
  • Jon M. Jenkins,
  • Avi Shporer,
  • Lyu ABE,
  • Philippe Bendjoya,
  • Jonathan L. Bush,
  • Marco Buttu,
  • Kevin I. Collins,
  • Jason D. Eastman,
  • Matthew J. Fields,
  • Thomas Gasparetto,
  • Maximilian N. Günther,
  • Veselin B. Kostov,
  • Adam L. Kraus,
  • Kathryn V. Lester,
  • Alan M. Levine,
  • Colin Littlefield,
  • Wenceslas Marie-Sainte,
  • Djamel Mékarnia,
  • Hugh P. Osborn,
  • David Rapetti,
  • George R. Ricker,
  • S. Seager,
  • Ramotholo Sefako,
  • Gregor Srdoc,
  • Olga Suarez,
  • Guillermo Torres,
  • Amaury H. M. J. Triaud,
  • R. Vanderspek,
  • Joshua N. Winn

DOI
https://doi.org/10.3847/1538-3881/acd197
Journal volume & issue
Vol. 165, no. 6
p. 268

Abstract

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We present the discovery and characterization of HIP 33609 b, a transiting warm brown dwarf orbiting a late B star, discovered by NASA's Transiting Exoplanet Survey Satellite as TOI-588 b. HIP 33609 b is a large ( R _b = ${1.580}_{-0.070}^{+0.074}$ R _J ) brown dwarf on a highly eccentric ( e = ${0.560}_{-0.031}^{+0.029}$ ) orbit with a 39 days period. The host star is a bright ( V = 7.3 mag), T _eff = 10,400 ${}_{-660}^{+800}$ K star with a mass of M _* = ${2.383}_{-0.095}^{+0.10}$ M _⊙ and radius of R _* = ${1.863}_{-0.082}^{+0.087}$ R _⊙ , making it the hottest transiting brown dwarf host star discovered to date. We obtained radial velocity measurements from the CHIRON spectrograph confirming the companion's mass of M _b = ${68.0}_{-7.1}^{+7.4}$ M _J as well as the host star's rotation rate ( $v\sin {i}_{* }=55.6\pm 1.8$ km s ^−1 ). We also present the discovery of a new comoving group of stars, designated as MELANGE-6, and determine that HIP 33609 is a member. We use a combination of rotation periods and isochrone models fit to the cluster members to estimate an age of 150 ± 25 Myr. With a measured mass, radius, and age, HIP 33609 b becomes a benchmark for substellar evolutionary models.

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