r-Process elements from magnetorotational hypernovae-Reference-Cited by-同舟云学术

r-Process elements from magnetorotational hypernovae

Published:2021-07-07 Issue:7866 Volume:595 Page:223-226
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Yong D.^ORCID,Kobayashi C.,Da Costa G. S.^ORCID,Bessell M. S.,Chiti A.^ORCID,Frebel A.^ORCID,Lind K.,Mackey A. D.^ORCID,Nordlander T.^ORCID,Asplund M.,Casey A. R.^ORCID,Marino A. F.,Murphy S. J.^ORCID,Schmidt B. P.^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/s41586-021-03611-2.pdf

Reference57 articles.

1. Ji, A. P., Frebel, A., Chiti, A. & Simon, J. D. r-Process enrichment from a single event in an ancient dwarf galaxy. Nature 531, 610–613 (2016).

2. Pian, E. et al. Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger. Nature 551, 67–70 (2017).

3. Kasen, D., Metzger, B., Barnes, J., Quataert, E. & Ramirez-Ruiz, E. Origin of the heavy elements in binary neutron-star mergers from a gravitational-wave event. Nature 551, 80–84 (2017).

4. Winteler, C. et al. Magnetorotationally driven supernovae as the origin of early galaxy r-process elements? Astrophys. J. 750, L22 (2012).

5. Haynes, C. J. & Kobayashi, C. Galactic simulations of r-process elemental abundances. Mon. Not. R. Astron. Soc. 483, 5123–5134 (2019).

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