We present projected rotational velocity values for 97 Galactic , 55 SMC , and 106 LMC O-B type stars from archival FUSE observations .
The evolved and unevolved samples from each environment are compared through the Kolmogorov-Smirnov test to determine if the distribution of equatorial rotational velocities is metallicity dependent for these massive objects .
Stellar interior models predict that massive stars with SMC metallicity will have significantly reduced angular momentum loss on the main sequence compared to their Galactic counterparts .
Our results find some support for this prediction but also show that even at Galactic metallicity , evolved and unevolved massive stars have fairly similar fractions of stars with large V \sin i values .
Macroturbulent broadening that is present in the spectral features of Galactic evolved massive stars is lower in the LMC and SMC samples .
This suggests the processes that lead to macroturbulence are dependent upon metallicity .