Star formation and accretion rates within 500 pc as traced by Gaia DR3 XP spectra

Open Access

Fig. F.1.

Plots of the fits used to derive the slopes of Fig. 15. Each is the fit is of a specific cluster of Sco-Cen, and the colours match those used in Fig. 15. The value of the slope of each region is reported. Fig. (a): log L_acc vs log L_⋆; Fig. (b): log Ṁ_acc vs log M_⋆.

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.