Where Are the M Dwarf Disks Older Than 10 Million Years?

We present 11.7-micron observations of nine late-type dwarfs obtained at theKeck I 10-meter telescope in December 2002 and April 2003. Our targets wereselected for their youth or apparent IRAS 12-micron excess. For all ninesources, excess infrared emission is not detected. We find that stellar winddrag can dominate the circumstellar grain removal and plausibly explain thedearth of M Dwarf systems older than 10 Myr with currently detected infraredexcesses. We predict M dwarfs possess fractional infrared excess on the orderof L_{IR}/L_{*}\sim10^{-6} and this may be detectable with future efforts.Comment: 24 pages, 2 figures, accepted to Ap