English

The VLT-FLAMES Tarantula Survey

Solar and Stellar Astrophysics 2017-11-15 v1 Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies Instrumentation and Methods for Astrophysics

Abstract

We present a number of notable results from the VLT-FLAMES Tarantula Survey (VFTS), an ESO Large Program during which we obtained multi-epoch medium-resolution optical spectroscopy of a very large sample of over 800 massive stars in the 30 Doradus region of the Large Magellanic Cloud (LMC). This unprecedented data-set has enabled us to address some key questions regarding atmospheres and winds, as well as the evolution of (very) massive stars. Here we focus on O-type runaways, the width of the main sequence, and the mass-loss rates for (very) massive stars. We also provide indications for the presence of a top-heavy initial mass function (IMF) in 30 Dor.

Keywords

Cite

@article{arxiv.1710.11220,
  title  = {The VLT-FLAMES Tarantula Survey},
  author = {Jorick S. Vink and C. J. Evans and J. Bestenlehner and C. McEvoy and O. Ramirez-Agudelo and H. Sana and F. Schneider and VFTS},
  journal= {arXiv preprint arXiv:1710.11220},
  year   = {2017}
}

Comments

7 Figures, 8 pages. Invited talk: IAUS 329: "The Lives and Death-Throes of Massive Stars"

R2 v1 2026-06-22T22:30:30.182Z