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The interplay between mass-loss and binarity

Published online by Cambridge University Press:  30 November 2022

Hugues Sana Open the ORCID record for Hugues Sana [Opens in a new window]
Hugues Sana*
Affiliation:
Institute of Astrophysics, KU Leuven, Celestijnlaan 200D, 3001 Leuven, Belgium email: hugues.sana@kuleuven.be
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Abstract

Most stars with birth masses larger than that of our Sun belong to binary or higher order multiple systems. Similarly, most stars have stellar winds. Radiation pressure and multiplicity create outflows of material that remove mass from the primary star and inject it into the interstellar medium or transfer it to a companion. Both have strong impact on the subsequent evolution of the stars, yet they are often studied separately. In this short review, I will sketch part of the landscape of the interplay between stellar winds and binarity. I will present several examples where binarity shapes the stellar outflows, providing new opportunities to understand and measure mass loss properties. Stellar winds spectral signatures often help clearly identifying key stages of stellar evolution. The multiplicity properties of these stages then shed a new light onto evolutionary connections between the different categories of evolved stars.

Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S366: The Origin of Outflows in Evolved Stars , November 2020 , pp. 83 - 95
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Copyright
© The Author(s), 2022. Published by Cambridge University Press on behalf of International Astronomical Union

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