Scott Kenyon: h-index, Total Citations, and Citation Map
Scott Kenyon's h-index is 100 (306 i10-index, 32,758+ total citations across 662+ publications) according to Google Scholar as of June 2026. Scott Kenyon is affiliated with Senior Scientist, Smithsonian Astrophysical Observatory.
Scott Kenyon is a researcher affiliated with Senior Scientist, Smithsonian Astrophysical Observatory, specializing in Astrophysics, Star & Planet Formation, Binary Stars. Their work has been cited 32,758 times. This profile visualizes their global influence, highlighting strong citation networks in Chile.
Scott Kenyon's Citation Metrics
Bibliometric impact based on 662 indexed publications. Of these, 4 are original research articles — the rest are literature highlights, conference abstracts or theses.
- H-Index
- 100
- i10-Index
- 306
- Total Citations
- 32,758
- Citing Countries
- 5
As of June 2026.
Scott Kenyon has an h-index of 100 and 32,758 total citations across 662 publications, with research cited by institutions in 5 countries.
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We've mapped 5,000 of 32,758 citations for Scott Kenyon
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Pre-main-sequence evolution in the Taurus-Auriga molecular cloud
19952,307
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Citation trend (last 10 years)Click to expand
Citation Trend (Last 10 Years)
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About Scott Kenyon's research
Scott Kenyon is a researcher in Astrophysics, Star & Planet Formation and Binary Stars at Senior Scientist, Smithsonian Astrophysical Observatory. Their work has been cited 32,758 times across 662 publications (h-index 100), according to Google Scholar.
Their most-cited work, “Pre-main-sequence evolution in the Taurus-Auriga molecular cloud” (1995), has accumulated 2,307 citations. Other influential works include “Spectral energy distributions of T Tauri stars-Disk flaring and limits on accretion” (1987) with 1,183 citations and “Annual Reviews Astron” (1996) with 797 citations.
Citations of Scott Kenyon's research come primarily from Chile, Germany and Netherlands, reflecting international research impact across 5+ countries. The interactive citation map above shows the full geographic distribution of the institutions citing this work.
