Open Access

Fig. 6

image

IR excess for all stars in sample at a specific phase is presented here, including (1) interpolated IR excess model from SPIPS, (see Sect. 2.2), (2) Spitzer observations stripped of various camera effects (see Sect. 2.3) and also corrected with regard to silicate absorption due to the ISM (orange curve, see Sect. 3.4).

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.