Hostname: page-component-78c5997874-xbtfd Total loading time: 0 Render date: 2024-11-20T01:34:02.696Z Has data issue: false hasContentIssue false
  • English
  • Français

Equilibrium structures of rapidly rotating stars with shellular rotation

Published online by Cambridge University Press:  28 July 2017

Kotaro Fujisawa  and
Yu Yamamoto
Kotaro Fujisawa
Affiliation:
Advanced Research Institute for Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku-ku, Tokyo 169-8555, Japan email: [email protected]
Yu Yamamoto
Affiliation:
Advanced Research Institute for Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku-ku, Tokyo 169-8555, Japan email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have developed a new numerical method for obtaining self-consistent structures of rapidly rotating stars. We obtained self-consistent equilibrium structures of rapidly rotating massive stars with shellular rotation by using the method. These equilibrium structures might be useful for both evolution of rapidly rotating massive stars and progenitor models of core-collapse supernovae simulations.

Keywords

stars: evolutionstars: rotation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S329: The Lives and Death-Throes of Massive Stars , November 2016 , pp. 398
Copyright
Copyright © International Astronomical Union 2017 

References

Fujisawa, K., 2015, MNRAS, 40, 1635 Google Scholar
Yamamoto, Y. & Yamada, S., 2016, ApJ, 818, 165 CrossRefGoogle Scholar