The Astronomical Journal (Jan 2024)

Direct-imaging Discovery of a Substellar Companion Orbiting the Accelerating Variable Star HIP 39017

  • Taylor L. Tobin,
  • Thayne Currie,
  • Yiting Li,
  • Jeffrey Chilcote,
  • Timothy D. Brandt,
  • Brianna Lacy,
  • Masayuki Kuzuhara,
  • Maria Vincent,
  • Mona El Morsy,
  • Vincent Deo,
  • Jonathan P. Williams,
  • Olivier Guyon,
  • Julien Lozi,
  • Sebastien Vievard,
  • Nour Skaf,
  • Kyohoon Ahn,
  • Tyler Groff,
  • N. Jeremy Kasdin,
  • Taichi Uyama,
  • Motohide Tamura,
  • Aidan Gibbs,
  • Briley L. Lewis,
  • Rachel Bowens-Rubin,
  • Maïssa Salama,
  • Qier An,
  • Minghan Chen

DOI
https://doi.org/10.3847/1538-3881/ad3077
Journal volume & issue
Vol. 167, no. 5
p. 205

Abstract

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We present the direct-imaging discovery of a substellar companion (a massive planet or low-mass brown dwarf) to the young, γ Doradus ( γ Dor)-type variable star HIP 39017 (HD 65526). The companion’s SCExAO/CHARIS JHK (1.1–2.4 μ m) spectrum and Keck/NIRC2 $L^{\prime} $ photometry indicate that it is an L/T transition object. A comparison of the JHK + L $^{\prime} $ spectrum to several atmospheric model grids finds a significantly better fit to cloudy models than cloudless models. Orbit modeling with relative astrometry and precision stellar astrometry from Hipparcos and Gaia yields a semimajor axis of ${23.8}_{-6.1}^{+8.7}$ au, a dynamical companion mass of ${30}_{-12}^{+31}$ M _J , and a mass ratio of ∼1.9%, properties most consistent with low-mass brown dwarfs. However, its mass estimated from luminosity models is a lower ∼13.8 M _J due to an estimated young age (≲115 Myr); using a weighted posterior distribution informed by conservative mass constraints from luminosity evolutionary models yields a lower dynamical mass of ${23.6}_{-7.4}^{+9.1}$ M _J and a mass ratio of ∼1.4%. Analysis of the host star’s multifrequency γ Dor-type pulsations, astrometric monitoring of HIP 39017 b, and Gaia Data Release 4 astrometry of the star will clarify the system age and better constrain the mass and orbit of the companion. This discovery further reinforces the improved efficiency of targeted direct-imaging campaigns informed by long-baseline, precision stellar astrometry.

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