Home > Science Articles > Non-refereed Articles > Mass-Loss Rates and Luminosities of Evolved Stars in the Magellanic Clouds |
published in EAS Publications Series, 71, pp. 57-64 (2015)
Abstract: I 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.
DOI: 10.1051/eas/1571011
Links: link
The record appears in these collections:
Royal Observatory of Belgium > Astronomy & Astrophysics
Science Articles > Non-refereed Articles