The splinter session proposed here aims to provide a venue for the
community studying circumstellar disks around cool stars and brown
dwarfs to: i, review the latest results from Spitzer, HST, and
ground-based facilities; ii, cast these results in a coherent
evolutionary sequence; iii, discuss the recent results and their
implications in detail, developing a better understanding of the
processes. The proposed session will be dominated by 15-minute
discussions on seven key topics: disk frequency and life time, disk
structure and mineralogy, disk masses, transition disks, planet
formation, and debris disks. Each topic will be introduced in a
10-minute review.
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