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Observing the mass-loss of nearby red supergiants through high-contrast imaging

Published online by Cambridge University Press:  30 December 2019

Peter Scicluna Open the ORCID record for Peter Scicluna [Opens in a new window] ,
R. Siebenmorgen ,
J. A. D. L. Blommaert ,
F. Kemper ,
R. Wesson  and
S. Wolf
Peter Scicluna
Affiliation:
Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), 11F Astronomy-Mathematics Building, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan email: peterscicluna@asiaa.sinica.edu.tw
R. Siebenmorgen
Affiliation:
ESO, Karl-Schwarzschild-Str. 2, 85748 Garching b. München, Germany
J. A. D. L. Blommaert
Affiliation:
Astronomy and Astrophysics Research Group, Dept. of Physics and Astrophysics, V.U. Brussel, Pleinlaan 2, 1050, Brussels, Belgium
F. Kemper
Affiliation:
Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), 11F Astronomy-Mathematics Building, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan email: peterscicluna@asiaa.sinica.edu.tw ESO, Karl-Schwarzschild-Str. 2, 85748 Garching b. München, Germany
R. Wesson
Affiliation:
Dept. of Physics & Astronomy, University College London, Gower Street, London WC1E 6BT, UK
S. Wolf
Affiliation:
ITAP, Universität zu Kiel, Leibnizstr. 15, 24118 Kiel, Germany
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Abstract

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We present observations of nearby red supergiants with SPHERE.

Keywords

stars: mass losscircumstellar matterstars: windsoutflows
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S343: Why Galaxies Care About AGB Stars: A Continuing Challenge through Cosmic Time , August 2018 , pp. 500 - 501
Copyright
© International Astronomical Union 2019 

References

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