Where Do Hot Jupiters Come from? Revisiting Tidal Disruption and Ejection in High-eccentricity Migration

Qianli 千里 Fan 范, Shang-Fei 尚飞 Liu 刘

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DOI: 10.3847/2041-8213/ae6659
Published: 2026-05-14
Container: The Astrophysical Journal Letters
Publisher: American Astronomical Society
Open access: unknown

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Cite this work

BibTeX

@article{allodium:10.3847/2041-8213/ae6659,
  title = {Where Do Hot Jupiters Come from? Revisiting Tidal Disruption and Ejection in High-eccentricity Migration},
  author = {Qianli 千里 Fan 范 and Shang-Fei 尚飞 Liu 刘},
  year = {2026},
  journal = {The Astrophysical Journal Letters},
  doi = {10.3847/2041-8213/ae6659},
  url = {https://doi.org/10.3847/2041-8213/ae6659}
}

RIS

TY  - JOUR
TI  - Where Do Hot Jupiters Come from? Revisiting Tidal Disruption and Ejection in High-eccentricity Migration
AU  - Qianli 千里 Fan 范
AU  - Shang-Fei 尚飞 Liu 刘
PY  - 2026
JO  - The Astrophysical Journal Letters
DO  - 10.3847/2041-8213/ae6659
UR  - https://doi.org/10.3847/2041-8213/ae6659
ER  -

APA

范, Q. 千. F., & 刘, S. 尚. L. (2026). Where Do Hot Jupiters Come from? Revisiting Tidal Disruption and Ejection in High-eccentricity Migration. The Astrophysical Journal Letters. https://doi.org/10.3847/2041-8213/ae6659

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crossref · retrieved 2026-11-10T11:40:13.621Z