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Neutron Star Mergers as the Main Source of r-process: Natal Kicks and Inside-out Evolution to the Rescue

  • Published:2020-10-19 Issue:2 Volume:902 Page:L34
  • ISSN:2041-8213
  • Container-title:The Astrophysical Journal
  • language:
  • Short-container-title:ApJ

Author:

Banerjee ProjjwalORCID,Wu Meng-RuORCID,Yuan ZhenORCID

Funder

Ministry of Science and Technology, Taiwan

Academia Sinica

Physics Division, National Center of Theoretical Science of Taiwan

LAMOST Fellow project

Shanghai Sailing Program

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 17 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. Location of the neutron drip line for Sn and its impact on r-process abundances;Physics Letters B;2024-08

2. How do nuclear isomers influence the gamma-ray bursts in binary neutron star mergers?;Frontiers in Astronomy and Space Sciences;2024-05-30

3. Decoding the compositions of four bright r-process-enhanced stars;Monthly Notices of the Royal Astronomical Society;2023-07-27

4. Origin of highly r-process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy;Monthly Notices of the Royal Astronomical Society;2022-11-14

5. Enrichment of the Galactic disc with neutron-capture elements: Gd, Dy, and Th;Monthly Notices of the Royal Astronomical Society;2022-08-25
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