Mass-loss rates in LMC and SMC O stars
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https://b2find.eudat.eu/dataset/e86a4ae5-a1f4-5cbf-8be5-77652ce396a0
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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...



