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Imaging Red Supergiants with VLT/SPHERE/ZIMPOL

Published online by Cambridge University Press:  30 December 2019

E. Cannon
Affiliation:
Instituut voor Sterrenkunde, KU Leuven, Leuven, Belgium email: [email protected]
M. Montargès
Affiliation:
Instituut voor Sterrenkunde, KU Leuven, Leuven, Belgium email: [email protected]
L. Decin
Affiliation:
Instituut voor Sterrenkunde, KU Leuven, Leuven, Belgium email: [email protected]
A. de Koter
Affiliation:
Instituut voor Sterrenkunde, KU Leuven, Leuven, Belgium email: [email protected] Anton Pannekoek Institute of Astronomy, University of Amsterdam, The Netherlands
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Abstract

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Using the VLT-SPHERE/ZIMPOL adaptive optics imaging polarimeter, images of a sample of nearby red supergiants (RSGs) were obtained in multiple filters. From these data, we obtain information on geometrical structures in the inner wind, the onset radius and spatial distribution of dust grains as well as dust properties such as grain size. As dust grains may play a role in initiating and/or driving the outflow, this could provide us with clues as to the wind driving mechanism.

Type
Contributed Papers
Copyright
© International Astronomical Union 2019 

References

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