  We present Keck/DEIMOS spectroscopy of resolved stars in the M31 satellites
And XXVIII & And XXIX. We show that these are likely self-bound galaxies based
on 18 and 24 members in And XXVIII & And XXIX, respectively. And XXVIII has a
systemic velocity of -331.1 +/- 1.8 km/s and velocity dispersion of 4.9+/-1.6
km/s, implying a mass-to-light ratio (within r_1/2) of ~ 44 +/- 41. And XXIX
has a systemic velocity of -194.4 +/- 1.5 km/s and velocity dispersion of
5.7+/-1.2 km/s, implying a mass-to-light ratio (within r_1/2) of ~ 124 +/- 72.
The internal kinematics and implied masses of And XXVIII & And XXIX are similar
to dwarf spheroidals (dSphs) of comparable luminosities, implying that these
objects are dark matter-dominated dwarf galaxies. Despite the large projected
distances from their host (380 and 188 kpc), the kinematics of these dSph
suggest that they are bound M31 satellites.
