Press Release
Free Access

Fig. 11

image

Star positions relative to gas for stars without Apogee RVs, i.e., the stars that are excluded from Fig. 7. We study these non-Apogee stars to determine whether the Apogee (Majewski et al. 2015; Da Rio et al. 2016) sample is systematically biased against stars lying within the dense spiny columns due to increased extinction. See Fig. 12. Ordinate is δ [deg].

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.