2017•Springer Link (Chiba Institute of Technology)Requires access
Mass-loss rates and luminosities of evolved stars in the Magellanic Clouds .
M. A. T. Groenewegen, G. C. Sloan
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Abstract
\nI describe how (dust) mass-loss rates and luminosities can be derived from fitting the SEDs of evolved stars in the Magellanic Clouds. I will discuss in more detail the influence of dust size, type and shape on the appearance of the dust features in the mid infra red.\n
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