Dynamical detection of a companion driving a spiral arm in a protoplanetary disk

Abstract

Radio and near-infrared observations have observed dozens of protoplanetary disks that host spiral arm features. Numerical simulations have shown that companions may excite spiral density waves in protoplanetary disks via companion–disk interaction. However, the lack of direct observational evidence for spiral-driving companions poses challenges to current theories of companion–disk interaction. Here we report multi-epoch observations of the binary system HD 100453 with the Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) facility at the Very Large Telescope. By recovering the spiral features via robustly removing starlight contamination, we measure spiral motion across 4 yr to perform dynamical motion analyses. The spiral pattern motion is consistent with the orbital motion of the eccentric companion. With this first observational evidence of a companion driving a spiral arm among protoplanetary disks, we directly and dynamically confirm the long-standing theory on the origin of spiral features in protoplanetary disks. With the pattern motion of companion-driven spirals being independent of companion mass, here we establish a feasible way of searching for hidden spiral-arm-driving planets that are beyond the detection of existing ground-based high-contrast imagers.

3C 273 host galaxy with Hubble Space Telescope coronagraphy

“…2.3.2, we used the median exposures from two stars as the empirical PSF template for 3C 273. Alternatively, the usage of archival data may better capture the PSFs of central sources to extract extended structures (e.g., Soummer et al 2014;Ren et al 2018;Sanghi et al 2022;Xie et al 2023). To explore this, we updated the coronagraphic PSF archive at the BAR5 location for STIS from Ren et al (2017).…”