SUBMILLIMETER CONSTRAINTS ON DUST NEAR LINDROOS POST T-TAURI STARS

Young stars from the dynamical sample identified by Lindroos [A&A, 156,223 (1986)] have been observe at 800 mum wavelength using the James Clerk Maxwell Telescope on Mauna Kea. The new data are used to constrain the mass of circumstellar dust around these stars. The Lindroos sample is dominated by low-mass stars of age (3-150)x10(6) yr, intermediate in age between the T Tauri and main-sequence stars. When combined with previous measurements, the present observations are compatible with the depletion of circumstellar dust on a time scale tau approximately 10(7.0) yr. If this dust is present in circumstellar disks, then tau represents the lifetime of these disks.