22 February 2021
The dust trails are composed of material from an encompassing nebula flowing into the disc. This nebula is likely the outcome of a collision between the star and a huge cloud of gas and dust, resulting in the unique shape of this planet-forming disc and the surrounding dust structure. A new study of SU Aur, which used the VLT and data from other telescopes, including the Atacama Large Millimeter/Submillimeter Array, showed that the nebula is still feeding material to the planet-forming disc. These new observations highlight how complex planet-forming discs can be.
Christian Ginski et al. Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Late infall causing disk misalignment and dynamic structures in SU Aur. In Astrophysical Journal Letters, February 18 2021.