| Issue |
EAS Publications Series
Volume 71-72, 2015
The Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau
|
|
|---|---|---|
| Page(s) | 57 - 64 | |
| Section | Winds, Mass Loss, Jets | |
| DOI | https://doi.org/10.1051/eas/1571011 | |
| Published online | 01 December 2015 | |
The Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau
E. Lagadec, F. Millour and T. Lanz (eds)
EAS Publications Series, 71–72 (2015) 57-64
E. Lagadec, F. Millour and T. Lanz (eds)
EAS Publications Series, 71–72 (2015) 57-64
Mass-Loss Rates and Luminosities of Evolved Stars in the Magellanic Clouds
Koninklijke Sterrenwacht van België, Ringlaan 3, 1180 Brussel, Belgium
e-mail: marting.groenewegen@oma.be
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.
© EAS, EDP Sciences, 2015