  Optical spectroscopic observations are reported for 24 and 23, nearby,
proper-motion-selected M-dwarf candidate members of the Beta Pictoris and AB
Doradus moving groups (BPMG and ABDMG). Using kinematic criteria, the presence
of both Halpha emission and high X-ray-to-bolometric luminosity, and position
in absolute colour-magnitude diagrams, 10 and 6 of these candidates are
confirmed as likely members of the BPMG and ABDMG respectively. Equivalent
widths or upper limits for the Li I 6708A line are reported and the lithium
depletion boundary (LDB) age of the BPMG is revisited. Whilst non-magnetic
evolutionary models still yield an estimated age of 21 +/- 4 Myr, models that
incorporate magnetic inhibition of convection imply an older age of 24 +/- 4
Myr. A similar systematic increase would be inferred if the stars were 25 per
cent covered by dark magnetic starspots. Since young, convective M-dwarfs are
magnetically active and do have starspots, we suggest that the original LDB age
estimate is a lower limit. The LDB age of the ABDMG is still poorly constrained
-- non-magnetic evolutionary models suggest an age in the range 35-150 Myr,
which could be significantly tightened by new measurements for existing
candidate members.

Solar and Stellar Astrophysics