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Be Star Disks: Powered by a Nonzero Central Torque

  • Published:2020-12-23 Issue:2 Volume:905 Page:L29
  • ISSN:2041-8213
  • Container-title:The Astrophysical Journal
  • language:
  • Short-container-title:ApJ

Author:

Nixon C. J.ORCID,Pringle J. E.

Funder

UKRI ∣ Science and Technology Facilities Council

EC ∣ Horizon 2020

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 9 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. To Be or Not To Be: The Role of Rotation in Modeling Galactic Be X-Ray Binaries;The Astrophysical Journal;2024-08-01

2. Decretion disc size in Be/X-ray binaries depends upon the disc aspect ratio;Monthly Notices of the Royal Astronomical Society;2024-05-02

3. Population synthesis of Be X-ray binaries: metallicity dependence of total X-ray outputs;Monthly Notices of the Royal Astronomical Society;2023-11-13

4. Disc precession in Be/X-ray binaries drives superorbital variations of outbursts and colour;Monthly Notices of the Royal Astronomical Society: Letters;2023-11-13

5. Ultraluminous X-ray sources;New Astronomy Reviews;2023-06
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