Impact of embedded circumplanetary winds on the circumstellar disk - I. Reshaping the local accretion environment

Open Access

Fig. 3

Estimated mass-loss rate, Ṁ_w, as a function of distance from the planet (in units of local scale height) for different A_γ values. The estimate assumes a volumetric density derived from a midplane surface density of Σ₀ = 40 g cm⁻² at R₀ = 10 AU.

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.