VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a "Failed Star"

Abstract

Young, low-mass Brown Dwarfs orbiting early-type stars, with low mass ratios (q≲0.01), appear intrinsically rare and present a formation dilemma: could a handful of these objects be the highest mass outcomes of “planetary” formation channels (bottom up within a protoplanetary disk), or are they more representative of the lowest mass “failed binaries” (formed via disk fragmentation, or core fragmentation)? Additionally, their orbits can yield model-independent dynamical masses, and when paired with wide wavelength coverage and accurate system age estimates, can constrain evolutionary models in a regime where the models have a wide dispersion depending on initial conditions. We present new interferometric observations of the 16Myr substellar companion HD136164Ab (HIP75056Ab) with VLTI/GRAVITY and an updated orbit fit including proper motion measurements from the Hipparcos-Gaia Catalogue of Accelerations. We estimate a dynamical mass of 35±10MJ (q∼0.02), making HD136164Ab the youngest substellar companion with a dynamical mass estimate. The new mass and newly constrained orbital eccentricity (e=0.44±0.03) and separation (22.5±1au) could indicate that the companion formed via the low-mass tail of the Initial Mass Function. Our atmospheric fit to the SPHINX M-dwarf model grid suggests a sub-solar C/O ratio of 0.45, and 3× solar metallicity, which could indicate formation in the circumstellar disk via disk fragmentation. Either way, the revised mass estimate likely excludes “bottom-up” formation via core accretion in the circumstellar disk. HD136164Ab joins a select group of young substellar objects with dynamical mass estimates; epoch astrometry from future Gaia data releases will constrain the dynamical mass of this crucial object further.

William Otto Balmer

Ph.D. Candidate

My research interests include distributed robotics, mobile computing and programmable matter.