Jul 25, 2022 · In addition, the outer spiral arm launched by the planet changes its pitch angle along the spiral due to the eccentricity and when it interacts ...
In this paper, we study the basic properties of vortex-driven spirals by the Rossby Wave Instability in 2D hydrodynamics simulations. We study how the surface ...
Jul 22, 2013 · SPIRAL STRUCTURE AND DIFFERENTIAL DUST SIZE DISTRIBUTION IN THE LkHα 330 DISK · E. AkiyamaJ. Hashimoto +58 authors. M. Tamura. Environmental ...
Dec 28, 2023 · While the depletion of dust in the inner disk and the appearance of spiral arms are enticing signposts of planet formation in disks, other ...
We investigate the spatial distribution of dust grains using a simple model of protoplanetary disk hosted by a giant gaseous vortex.
Mar 10, 2023 · The relative gas surface density profile inside the dust cavity can be determined using ALMA CO isotopologue data, with sufficient resolution to ...
There is much evidence that planet formation is occurring in the disc around the Herbig. Be star HD100546. To learn more about the processes occurring in ...
Spiral Structure and Differential Dust Size Distribution in the LkH(alpha) 330 Disk ... differential dust size distribution between the two sides of the disk.
Mid-infrared spectrophotometric observations have revealed a small sub-class of circumstellar disks with spectral energy distributions (SEDs) suggestive of ...
Missing: SPIRAL DIFFERENTIAL SIZE