Mass-loss rates in LMC and SMC O stars

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...我们结合BVJHK测光数据与斯皮策（Spitzer）空间望远镜的3.6、5.8及8.0微米测光数据，对包含58个大麦哲伦云（Large Magellanic Cloud）源与46个小麦哲伦云（Small Magellanic Cloud）源的样本开展红外超（infrared excess, IR）的判定工作。