Free Access

Fig. 4

thumbnail

Variations of dust production rates by AGB stars for silicate, carbonaceous, SiC, and iron dust during the LMC evolution calculated with dust yields taken from Zhukovska et al. (2008). The DPR for silicates and carbonaceous grains from SN II are shown for illustration. The production rate for metallic iron by SN II is added to that of silicates. Uncertainties in DPR for each species due to the uncertainties in the SFH fit are shown as shaded regions. Open and closed symbols show the current DPRs for carbon- and oxygen-rich dust, respectively, derived from IR observations by Matsuura et al. (2009, triangles, with an arrow marking an upper limit), Boyer et al. (2012, squares), Riebel et al. (2012, circles), and Srinivasan et al. (2009, diamonds).

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.