Fig. 10
Download original image
X-ray versus bolometric luminosity for the WR stars in Wd1. The top panel depicts the “classical” correlation using the 0.5–8.0 keV band in the X-rays, while the bottom panel shows the same correlation using the 4–8.0 keV X-ray band. Upper limits on X-ray-undetected WR stars are shown with black triangles. X-ray luminosities are obtained using solar abundances.
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.