RZ Psc is a young Sun-like star with a bright and warm infrared excess that is occasionally dimmed significantly by circumstellar dust structures. Optical depth arguments suggest that the dimming events do not probe a typical sight line through the circumstellar dust, and are instead caused by structures that appear above an optically thick mid-plane. This system may therefore be similar to systems where an outer disk is shadowed by material closer to the star. Here we report the discovery that RZ Psc hosts a 0.12M⊙ companion at a projected separation of 23au. We conclude that the disk must orbit the primary star. While we do not detect orbital motion, comparison of the angle of linear polarization of the primary with the companion's on-sky position angle provides circumstantial evidence that the companion and disc may not share the same orbital plane. Whether the companion severely disrupts the disc, truncates it, or has little effect at all, will require further observations of both the companion and disc.
@article{arxiv.2005.14203,
title = {A low-mass stellar companion to the young variable star RZ Psc},
author = {Grant M. Kennedy and Christian Ginski and Matthew A. Kenworthy and Myriam Benisty and Thomas Henning and Rob G. van Holstein and Quentin Kral and François Ménard and Julien Milli and Luis Henry Quiroga-Nuñez and Christian Rab and Tomas Stolker and Ardjan Sturm},
journal= {arXiv preprint arXiv:2005.14203},
year = {2020}
}