Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
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doi.org/10.1086/341728 →Countries where authors are citing Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
This map shows the geographic impact of Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics more than expected).
Fields of papers citing Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
This network shows the impact of Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics.
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.
This paper is also available at doi.org/10.1086/341728.