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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

Abstract

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

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