A lanthanide-rich kilonova in the aftermath of a long gamma-ray burst-Reference-Cited by-同舟云学术

A lanthanide-rich kilonova in the aftermath of a long gamma-ray burst

Published:2024-02-21 Issue:8000 Volume:626 Page:742-745
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Yang Yu-Han^ORCID,Troja Eleonora^ORCID,O’Connor Brendan^ORCID,Fryer Chris L.^ORCID,Im Myungshin^ORCID,Durbak Joe,Paek Gregory S. H.^ORCID,Ricci Roberto,Bom Clécio R.^ORCID,Gillanders James H.,Castro-Tirado Alberto J.^ORCID,Peng Zong-Kai,Dichiara Simone,Ryan Geoffrey^ORCID,van Eerten Hendrik,Dai Zi-Gao,Chang Seo-Won^ORCID,Choi Hyeonho^ORCID,De Kishalay^ORCID,Hu Youdong,Kilpatrick Charles D.^ORCID,Kutyrev Alexander,Jeong Mankeun^ORCID,Lee Chung-Uk^ORCID,Makler Martin,Navarete Felipe,Pérez-García Ignacio

Publisher

Springer Science and Business Media LLC

Link

https://www.nature.com/articles/s41586-023-06979-5.pdf

Reference72 articles.

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3. Freiburghaus, C., Rosswog, S. & Thielemann, F. K. R-process in neutron star mergers. Astrophys. J. 525, L121–L124 (1999).

4. Korobkin, O., Rosswog, S., Arcones, A. & Winteler, C. On the astrophysical robustness of the neutron star merger r-process. Mon. Not. R. Astron. Soc. 426, 1940–1949 (2012).

5. Barnes, J., Kasen, D., Wu, M.-R. & Martínez-Pinedo, G. Radioactivity and thermalization in the ejecta of compact object mergers and their impact on kilonova light curves. Astrophys. J. 829, 110 (2016).

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