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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.

preprint2011arXivOpen access
P. L. DuftonP. R. DunstallC. J. EvansI. BrottM. CantielloA. de KoterS. E. de MinkM. FraserV. Hénault-BrunetI. D. HowarthN. LangerD. J. LennonN. MarkovaH. SanaW. D. Taylor
astro-ph.SR
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P. L. DuftonP. R. DunstallC. J. EvansI. BrottM. CantielloA. de KoterS. E. de MinkM. FraserV. Hénault-BrunetI. D. HowarthN. LangerD. J. LennonN. MarkovaH. SanaW. D. Taylor

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