Modeling the astrosphere of LHS 1140 - On the differences of 3D magnetohydrodynamic single- and multi-fluid simulations and the consequences for exoplanetary habitability

Open Access

Fig. 8

TS, AP, and BS distance changes caused by different stellar wind speeds: υ_sw = 250km/s (black line) and υ_sw = 1000 km/s (red line). In both runs a stellar mass-loss rate of Ṁ = 1.2 · 10⁻¹⁵ M_⊙/yr was assumed. The blue line shows the distances for υ_sw = 430 km/s and Ṁ = 2.6 · 10⁻¹⁶ M_⊙/yr.

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.