A three-dimensional hydrodynamics simulation of oxygen-shell burning in the 
final evolution of a fast-rotating massive star

Yoshida, Takashi; Takiwaki, Tomoya; Aguilera-Dena, David R.; Kotake, Kei; Takahashi, Koh; Nakamura, Ko; Umeda, Hideyuki; Langer, Norbert

doi:10.1093/mnrasl/slab067

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A three-dimensional hydrodynamics simulation of oxygen-shell burning in the final evolution of a fast-rotating massive star

Yoshida, T., Takiwaki, T., Aguilera-Dena, D. R., Kotake, K., Takahashi, K., Nakamura, K., et al. (2021). A three-dimensional hydrodynamics simulation of oxygen-shell burning in the final evolution of a fast-rotating massive star. \mnras, 506(1), L20-L25. doi:10.1093/mnrasl/slab067.

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Item Permalink: https://hdl.handle.net/21.11116/0000-000A-728F-5 Version Permalink: https://hdl.handle.net/21.11116/0000-000A-7290-2

Genre: Journal Article

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Creators:
Yoshida, Takashi, Author
Takiwaki, Tomoya, Author
Aguilera-Dena, David R., Author
Kotake, Kei, Author
Takahashi, Koh, Author
Nakamura, Ko, Author
Umeda, Hideyuki, Author
Langer, Norbert¹, Author

Affiliations:
1Max Planck Institute for Radio Astronomy, Max Planck Society, ou_2205652

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Free keywords: convection, hydrodynamics, stars: massive, stars: rotation, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena

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Dates: Date issued: 2021-09

Publication Status: Issued

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Identifiers: DOI: 10.1093/mnrasl/slab067
BibTex Citekey: 2021MNRAS.506L..20Y

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Title: \mnras

Source Genre: Journal

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Pages: - Volume / Issue: 506 (1) Sequence Number: - Start / End Page: L20 - L25 Identifier: -