Work

Nucleosynthesis of Pop III and Fe-enriched Pop II pair-instability supernovae

Year: 2026

Type: article

Source: Science China Physics Mechanics and Astronomy

DOI: 10.1007/s11433-026-3079-x

Authors: Wenyu Xin, Ken’ichi Nomoto, Chun-Ming Yip, Xianfei Zhang, Qian-Fan Xing, Shaolan Bi, Gang Zhao

Institutions: Beijing Normal University, Kavli Institute for the Physics and Mathematics of the Universe, The University of Tokyo Institutes for Advanced Study, GSI Helmholtz Centre for Heavy Ion Research, Chinese University of Hong Kong, Chinese Academy of Sciences, National Astronomical Observatories, University of Chinese Academy of Sciences

Language: English

Topic: Gamma-ray bursts and supernovae

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: green

Funders: European Commission, Ministry of Education, Culture, Sports, Science and Technology, National Natural Science Foundation of China, Chinese Academy of Sciences, Japan Society for the Promotion of Science

Awards: G1682633203, G215699715, G271529020, G5073340295, G6231484428, Exploring the evolution and nucleosynthesis of massive stars and Galactic chemical evolution through nitrogen abundances in early generations of stars, G680404248, G7082738492, G7770810943, 極低金属銀河や遠方クエーサーの鉄の大量生成源が極超新星か電子対生成超新星かの解明

OpenAlex ID: W7168250049

FWCI:

Cites: 81

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Related to: 10