The VLT-FLAMES Tarantula Survey: The fastest rotating O-type star and   shortest period LMC pulsar - remnants of a supernova disrupted binary?
  We present a spectroscopic analysis of an extremely rapidly rotating late O-type star, VFTS102, observed during a spectroscopic survey of 30 Doradus. VFTS102 has a projected rotational velocity larger than 500\kms\ and probably as large as 600\kms; as such it would appear to be the most rapidly rotating massive star currently identified. Its radial velocity differs by 40\kms\ from the mean for 30 Doradus, suggesting that it is a runaway. VFTS102 lies 12 pcs from the X-ray pulsar PSR J0537-6910 in the tail of its X-ray diffuse emission. We suggest that these objects originated from a binary system with the rotational and radial velocities of VFTS102 resulting from mass transfer from the progenitor of PSR J0537-691 and the supernova explosion respectively. 
P. L. Dufton, P. R. Dunstall, C. J. Evans, I. Brott, M. Cantiello, A.   de Koter, S.E. de Mink, M. Fraser, V. H\'enault-Brun...
astro-ph.SR