  This paper continues the analysis of faint high latitude B stars from Martin
(2004). Here we analyze the kinematics of the stars and combine them with the
abundance information from the first paper to classify each one. The sample
contains 31 Population I runaways, fifteen old evolved stars (including five
BHB stars, three post-HB stars, a pulsating helium dwarf, and six stars of
ambiguous classification), one F-dwarf, and two stars which do not easily fit
in one of the other categories. No star in the sample unambiguously shows the
characteristics of a young massive star formed in situ in the halo. The two
unclassified stars are probably extreme Population I runaways. The low binary
frequency and rotational velocity distribution of the Population I runaways
imply that most were ejected from dense star clusters by DES (dynamic ejection
scenario). However we remain puzzled by the lack of runaway Be stars. We also
confirm that PB 166 and HIP 41979 are both nearby solar-metallicity BHB stars.
