James W. Johnson
Physics and Astronomy · The Ohio State University
Publications
264
Citations
6,973
Est. group size
~4
Recurring co-author estimate
Active years
60
Publishing since 1967
James W. Johnson studies how the Milky Way galaxy's chemical composition has evolved over cosmic time, using large surveys of stars to trace patterns of elements like carbon, nitrogen, and helium. This work, often called 'galactic chemical evolution' or 'galactic archaeology,' helps reconstruct the history of star formation and how different parts of the galaxy formed and merged. Prospective students would likely work with large public datasets from sky surveys such as SDSS and APOGEE, combining observational data analysis with modeling of stellar processes.
Publication output has grown substantially over the last decade, rising from just a few papers per year around 2017-2019 to a sustained pace of roughly 8-11 papers annually since 2021.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- [C/N] Ages for Red Giants and Their Implications for Galactic Archaeology
The Astrophysical Journal · 2026
- Milky Way Mapper decoded abundances – I. Shared disc enrichment patterns
Monthly Notices of the Royal Astronomical Society · 2026
- Search for β-delayed fission of Aug,m178 and an updated systematics in the region of neutron-deficient nuclei
HAL (Le Centre pour la Communication Scientifique Directe) · 2026
- The galactic chemical evolution of carbon: implications for stellar nucleosynthesis
Monthly Notices of the Royal Astronomical Society · 2026
- A Galactic Perspective on the (Unremarkable) Relative Refractory Depletion Observed in the Sun
The Astrophysical Journal · 2026
- Towards a measurement of the primordial helium isotope ratio
Apollo (University of Cambridge) · 2026
- Milky Way Mapper decoded abundances – II. From patterns to paths
Monthly Notices of the Royal Astronomical Society · 2026
- Towards a Measurement of the Primordial Helium Isotope Ratio*
The Astrophysical Journal · 2026
- Scylla at APOGEE: The Impact of Starbursts on the Chemical Evolution of the Magellanic Clouds
The Astrophysical Journal · 2026
- The Nineteenth Data Release of the Sloan Digital Sky Survey
The Astrophysical Journal Supplement Series · 2026
- The Milky Way Radial Metallicity Gradient as an Equilibrium Phenomenon: Why Old Stars Are Metal Rich
The Astrophysical Journal · 2025
- Many Elements Matter: Detailed Abundance Patterns Reveal Star Formation and Enrichment Differences among Milky Way Structural Components
The Astronomical Journal · 2025
- Modelling the Galactic Chemical Evolution of Helium
Monthly Notices of the Royal Astronomical Society · 2025
- Rising from the Ashes. II. The Bar-driven Abundance Bimodality of the Milky Way
The Astrophysical Journal · 2025
- The Open Cluster Chemical Abundances and Mapping Survey: VIII. Galactic Chemical Gradient and Azimuthal Analysis from SDSS/MWM DR19
arXiv (Cornell University) · 2025
- arXiv (Cornell University)×17
- Monthly Notices of the Royal Astronomical Society×12
- The Astrophysical Journal×12
- Physical Review C×5
- The Astrophysical Journal Supplement Series×2
- B. Scott Gaudi
Physics and Astronomy · The Ohio State University
- Andrew Gould
Physics and Astronomy · The Ohio State University
- Alison Duck
Physics and Astronomy · The Ohio State University
- Adam Wheeler
Physics and Astronomy · The Ohio State University
- Byeong-Gon Park
Physics and Astronomy · The Ohio State University
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 19, 2026.
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