The parallaxes of eight galactic X-ray sources measured by Hipparcos are co
nsistent with zero in all but two cases, 4U1145-619 (= Cen X-5) and HZ43. T
he parallax and proper motion measured for each of the others, including th
e Be/neutron star binaries X Per and A0535+26 and the massive X-ray binarie
s 4U0900-40, 4U1700-37, and Cyg XR-1, are consistent with their spectroscop
ic parallaxes. These results provide no evidence that visible stars in X-ra
y binaries have a luminosity that is abnormal for their spectral type.