Space astrometry of the very massive ∼150 M⊙ candidate runaway star VFTS682

@article{Renzo2018SpaceAO,
  title={Space astrometry of the very massive ∼150 M⊙ candidate runaway star VFTS682},
  author={Mathieu Renzo and Selma E de Mink and Daniel J. Lennon and Imants Platais and Roeland P van der Marel and Eva Laplace and Joachim M. Bestenlehner and C. J. Evans and Vincent H'enault-Brunet and Stephen Justham and Alex de Koter and Norbert Langer and Francisco Najarro and Fabian R. N. Schneider and Jorick S. Vink},
  journal={Monthly Notices of the Royal Astronomical Society: Letters},
  year={2018}
}
How very massive stars form is still an open question in astrophysics. VFTS682 is among the most massive stars known, with an inferred initial mass of ≳150M⊙⁠. It is located in 30 Doradus at a projected distance of 29 pc from the central cluster R136. Its apparent isolation led to two hypotheses: either it formed in relative isolation or it was ejected dynamically from the cluster. We investigate the kinematics of VFTS682 as obtained by Gaia and Hubble Space Telescope astrometry. We derive a… 

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