Planets around evolved intermediate-mass stars - II. Are there really planets around IC 4651 No. 9122, NGC 2423 No. 3, and NGC 4349 No. 127?

Free Access

Fig. 11

Radial velocity data as a function of time for NGC 4349 No. 127. The fitted orbit corresponds to a period of 672 days. A stellar jitter of 15 m s⁻¹ has been added to the error bars.

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.