Volume 570, October 2014
|Number of page(s)||10|
|Section||Planets and planetary systems|
|Published online||30 October 2014|
We present the numerical results of this study for the full Bcool sample.
Ram pressure, Pram, exerted on a hypothetical Earth analogue located in the centre of the habitable zone, rHZ, the corresponding magnetospheric size, rMP, and the mass-loss rates, Ṁ, for the Bcool sample of stars.
© ESO, 2014
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.