A geometric distance to the galaxy NGC4258 from orbital motions in a nuclear gas disk
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This map shows the geographic impact of A geometric distance to the galaxy NGC4258 from orbital motions in a nuclear gas disk. 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 A geometric distance to the galaxy NGC4258 from orbital motions in a nuclear gas disk with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A geometric distance to the galaxy NGC4258 from orbital motions in a nuclear gas disk more than expected).
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This network shows the impact of A geometric distance to the galaxy NGC4258 from orbital motions in a nuclear gas disk. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the A geometric distance to the galaxy NGC4258 from orbital motions in a nuclear gas disk.
About A geometric distance to the galaxy NGC4258 from orbital motions in a nuclear gas disk
This paper, published in 1999, received 238 indexed citations . Written by J. R. Herrnstein, J. M. Moran, L. J. Greenhill, P. J. Diamond, Makoto Inoue, Naomasa Nakai, Makoto Miyoshi, C. Henkel and Adam G. Riess covering the research area of Nuclear and High Energy Physics and Astronomy and Astrophysics. It is primarily cited by scholars working on Astronomy and Astrophysics (235 citations), Nuclear and High Energy Physics (70 citations) and Instrumentation (38 citations). Published in Nature.
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This paper is also available at doi.org/10.1038/22972.