Fig. 17
Molecular fraction versus neutral atomic-hydrogen column density for the GRB-DLAs from this paper and Ledoux et al. (2009) and Prochaska et al. (2009) compared to QSO-DLAs (Noterdaeme et al. 2008, 2015a; Balashev et al. 2017; Ranjan et al. 2018) and Galactic sight-lines probing diffuse and translucent clouds (Burgh et al. 2010). H2 -bearing DLAs are plotted with colored symbols and the non-detections in gray. For GRB 120327A, 120909A, and 141109A, we plot the molecular fraction for both b = 2 and b = 10 km s−1.
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.