Mass-loss rates from mid-infrared excesses in LMC and SMC O stars

@article{Massa2017MasslossRF,
  title={Mass-loss rates from mid-infrared excesses in LMC and SMC O stars},
  author={D. L. Massa and Alex W. Fullerton and Raman K. Prinja},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2017},
  volume={470},
  pages={3765-3774}
}
We use a combination of BVJHK and Spitzer [3.6], [5.8] and [8.0] photometry to determine infrared (IR) excesses for a sample of 58 Large Magellanic Cloud and 46 Small Magellanic Cloud O stars. This sample is ideal for determining IR excesses because the very small line-of-sight reddening minimizes uncertainties due to extinction corrections. We use the core–halo model developed by Lamers & Waters to translate the excesses into mass-loss rates and demonstrate that the results of this simple… 
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