Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars
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doi.org/10.1086/149707 →Countries where authors are citing Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars
This map shows the geographic impact of Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars. 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 Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars more than expected).
Fields of papers citing Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars
This network shows the impact of Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars.
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This paper is also available at doi.org/10.1086/149707.