Planet Formation Around M-dwarfs: From Young Disks to Planets
  Cool M dwarfs outnumber sun-like G stars by ten to one in the solar neighborhood. Due to their proximity, small size, and low mass, M-dwarf stars are becoming attractive targets for exoplanet searches via almost all current search methods. But what planetary systems can form around M dwarfs? Following up on the Cool Stars~16 Splinter Session "Planet Formation Around M Dwarfs", we summarize here our knowledge of protoplanetary disks around cool stars, how they disperse, what planetary systems might form and can be detected with current and future instruments. 
I. Pascucci, G. Laughlin, B. S. Gaudi, G. Kennedy, K. Luhman, S.   Mohanty, J. Birkby, B. Ercolano, P. Plavchan, A. Skemer
astro-ph.EP