Open Access

Fig. 3.

image

Download original image

Distribution of the additional total proper motions (Δμ) and their significance (Δμ/σμ) caused by secular aberration drift due to the change in the line of sight for Galactic stars with a total proper motion exceeding 1 mas yr−1. (a) Scatter plot of Δμ versus Δμ/σμ. The ten sources with the greatest additional proper motion are highlighted, with their names labeled near the data points. (b) Histogram of Δμ. (c) Histogram of Δμ/σμ.

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.