Azimuthal asymmetries in the debris disk around HD 61005
Azimuthal asymmetries in the debris disk around HD 61005
Debris disks offer valuable insights into the latest stages of circumstellar disk evolution, and can possibly help us to trace the outcomes of planetary formation processes. In the age range 10 to 100\,Myr, most of the gas is expected to have been removed from the system, giant planets (if any) …