Contact Tracing of Massive Binary Stars

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Abstract:

Stellar mergers produce more massive, rejuvenated (strongly magnetic) stars, with potentially peculiar properties, and can be detected as luminous red novae. Using a grid of detailed 1D binary evolution models, we aim to determine which binary systems are likely to merge and at what evolutionary stage. This will tell us more about the merger products, and might help us understand some of the trends found in observed single- and multiple-star populations.

SEEK ID: https://publications.h-its.org/publications/2056

DOI: 10.1017/S1743921322002708

Research Groups: Theory and Observations of Stars

Publication type: Journal

Journal: Proceedings of the International Astronomical Union

Citation: Proc. IAU 18(S361):311-312

Date Published: 1st May 2022

Registered Mode: by DOI

Authors: Jan Henneco, Fabian R. N. Schneider, Saskia Hekker, Eva Laplace

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Kristin Weidner

Citation

Henneco, J., Schneider, F. R. N., Hekker, S., & Laplace, E. (2022). Contact Tracing of Massive Binary Stars. In Proceedings of the International Astronomical Union (Vol. 18, Issue S361, pp. 311–312). Cambridge University Press (CUP). https://doi.org/10.1017/s1743921322002708

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Created: 11th Apr 2025 at 09:26

Last updated: 11th Apr 2025 at 09:27

Contact Tracing of Massive Binary Stars

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