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Near and far: a hunt for binary-interaction products

Published online by Cambridge University Press:  29 August 2024

J. Bodensteiner*
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str. 2, 85738 Garching bei M/"unchen, Germany Institute for Astronomy, KU Leuven, Celestijnenlaan 200 D, 3001, Leuven, Belgium
H. Sana
Affiliation:
Institute for Astronomy, KU Leuven, Celestijnenlaan 200 D, 3001, Leuven, Belgium
L. Mahy
Affiliation:
Royal Observatory of Belgium, Avenue Circulaire 3, B-1180 Brussel, Belgium
T. Shenar
Affiliation:
Anton Pannekoek Institute for Astronomy, University of Amsterdam, Postbus 94249, 1090 GE Amsterdam, The Netherlands
G. Banyard
Affiliation:
Institute for Astronomy, KU Leuven, Celestijnenlaan 200 D, 3001, Leuven, Belgium
C. Wang
Affiliation:
Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str. 1, 85748 Garching, Germany
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Abstract

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Direct observations of the products of binary interactions are sparse, yet they provide important insights on the outcome of the interaction and the physics at play. Young and intermediate-age star clusters are the ideal tool to search for, and characterize such interaction products and allow for a detailed comparison to theoretical predictions. We here report on integral field spectroscopy obtained with MUSE for several such clusters in the Magellanic Clouds.

Type
Poster Paper
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

References

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