The
one galactic ``relativistic jet'' known in 1984 was
SS433, with outflow at 0.26
. Cygnus
X-3 has since hinted of expansion at about /3 (Spencer
et al. 1986; Schalinski et al. 1995), though its kinematics and distance
are ambiguous. As noted by Scheuer (these Proceedings),
stronger candidates for the ``mini-quasar'' appellation have surfaced in the
X-ray transients GRS1915+105 (Mirabel &
Rodríguez 1994) and GROJ1655-40 (Tingay
et al. 1995; Hjellming & Rupen 1995), both with relativistic pattern
speeds approaching those of quasars. The galactic 
-ray
sources 1E1740.7-2942 (Mirabel et al. 1992)
and GRS1758-258 (Rodríguez, Mirabel, &
Martí 1992) also show signs of jet-like radio structure, though
nothing is known of their proper motions. The validity of calling all such
sources ``mini-quasars'' is unclear, but studying their (rapid)
evolution may well illuminate the AGN-jet problem.