Work

Azimuthal asymmetries in the debris disk around HD 61005

Year: 2016
Type: article
Abstract: Context. 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) must have already been formed, and the formation of terrestrial planets may be on-going. Pluto-sized planetesimals, and their debris released in a collisional cascade, are under their mutual gravitational influence, which may result into non-axisymmetric structures in the debris disk.
Language: English
Open Access status: bronze
Award: G753270600
OpenAlex ID: W2372770452
FWCI: 6.469
Cites: 116
Cited by: 103
Related to: 10