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

Abstract

We present the direct-imaging discovery of a substellar companion (a massive planet or low-mass brown dwarf) to the young, ${\hat{I}}^3$ Doradus-type variable star, HIP 39017 (HD 65526). The companion's SCExAO/CHARIS JHK ($1.1-2.4\hat{I}¼$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 semi-major axis of $23.8_{-6.1}^{+8.7}$ au, a dynamical companion mass of $30_{-12}^{+31}$~M${}_J$, and a mass ratio of $\sim$1.9\%, properties most consistent with low-mass brown dwarfs. However, its mass estimated from luminosity models is a lower $\sim$13.8 $M_{\mathrm{J}}$ due to an estimated young age ($\lesssim$ 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 $\sim$1.4\%. Analysis of the host star's multi-frequency ${\hat{I}}^3$ Dor-type pulsations, astrometric monitoring of HIP 39017b, 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.

Published in AJ: April 9, 2024