Constraints on the multiplicity of the most massive stars known: R136 a1, a2, a3, and c

Shenar, T. orcid.org/0000-0003-0642-8107, Sana, H., Crowther, P.A. et al. (5 more authors) (2023) Constraints on the multiplicity of the most massive stars known: R136 a1, a2, a3, and c. Astronomy & Astrophysics, 679. A36. ISSN 0004-6361

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Item Type: Article
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© The Authors 2023. Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Keywords: stars: Wolf–Rayet; binaries: spectroscopic; stars: massive; Magellanic Clouds
Dates:
  • Published: November 2023
  • Published (online): 1 November 2023
  • Accepted: 21 September 2023
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Funding Information:
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Grant number
SCIENCE AND TECHNOLOGY FACILITIES COUNCIL
ST/V000853/1
Depositing User: Symplectic Sheffield
Date Deposited: 18 Jan 2024 13:52
Last Modified: 18 Jan 2024 13:52
Status: Published
Publisher: EDP Sciences
Refereed: Yes
Identification Number: 10.1051/0004-6361/202346930
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