The Parallax of VHS J1256-1257 from CFHT and Pan-STARRS 1

Abstract

We present new parallax measurements from the CFHT Infrared Parallax Program and the Pan-STARRS 3π Steradian Survey for the young (≈150−300 Myr) triple system VHS J125601.92−125723.9. This system is composed of a nearly equal-flux binary ("AB") and a wide, possibly planetary-mass companion ("b"). The system's published parallactic distance (12.7±1.0 pc) implies absolute magnitudes unusually faint compared to known young objects and is in tension with the spectrophotometric distance for the central binary (17.2±2.6 pc). Our CFHT and Pan-STARRS parallaxes are consistent, and the more precise CFHT result places VHS J1256-1257 at 22.2+1.1−1.2 pc. Our new distance results in higher values for the companion's mass (19±5 MJup) and temperature (1240±50 K), and also brings the absolute magnitudes of all three components into better agreement with known young objects.