Magnetic clumping of charged dust in the dense interstellar medium

Open Access

Fig. 3

Schematic illustration of the parameters controlling the transverse-to-longitudinal magnetic field ratio $B_{⊥} / B_{∥}$ $B_{\perp} / B_{\|}$ and thus the intensity of dust clumping via the parametric instability in the simulations with turbulence.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.