Smita Mathur
Physics and Astronomy · The Ohio State University
Publications
341
Citations
7,366
Est. group size
~4
Recurring co-author estimate
Active years
46
Publishing since 1981
Smita Mathur's research focuses on the hot, diffuse gas surrounding galaxies (the circumgalactic medium) and the interstellar medium of the Milky Way and other galaxies, studied largely through X-ray observations. Related work examines active galactic nuclei (AGN) and the supermassive black holes that power them, including their winds and disc structure, as well as star cluster formation in galaxies. The work relies heavily on space-based X-ray telescopes and multi-wavelength data (including ALMA, HST, and JWST) to trace gas properties, temperature, and chemical composition across galactic and intergalactic environments.
Publication output was fairly steady at 6-8 papers per year from 2017-2021, then increased notably to 13-16 papers per year in 2022-2024, with a decline in the most recent partial years.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- The nuclear star cluster of M 74: A fossil record of the very early stages of a star-forming galaxy
Astronomy and Astrophysics · 2026
- Erratum: “Thermal Sunyaev–Zel’dovich Effect in the Circumgalactic Medium. II. Dependence on Star Formation” (2025, ApJ, 991, 205)
The Astrophysical Journal · 2026
- Thermal Sunyaev–Zel’dovich Effect in the Circumgalactic Medium. II. Dependence on Star Formation
The Astrophysical Journal · 2025
- Departures from standard disc predictions in intensive ground-based monitoring of three AGNs
Monthly Notices of the Royal Astronomical Society · 2025
- Where is the Supervirial Gas? The Supply from Hot Inflows
The Astrophysical Journal · 2025
- Where is the Supervirial Gas? II. Insight from the Survey of Galactic Sightlines
The Astrophysical Journal · 2025
- Where Is the Supervirial Gas? III. Insights from X-Ray Shadow Observations and a Revised Model for the Soft Diffuse X-Ray Background
The Astrophysical Journal · 2025
- Where is the Supervirial Gas? III. Insights from X-ray Shadow Observations and a revised Model for the Soft Diffuse X-ray Background
arXiv (Cornell University) · 2025
- Hidden Gems on a Ring: Infant Massive Clusters and Their Formation Timeline Unveiled by ALMA, HST, and JWST in NGC 3351
The Astrophysical Journal · 2024
- Supermassive Black Hole Winds in X-rays: SUBWAYS
Astronomy and Astrophysics · 2024
- <i>XMM–Newton</i> Ultra Narrow Deep Field survey – II. X-ray spectral analysis of the brightest AGN population
Monthly Notices of the Royal Astronomical Society · 2024
- On the Origin of the 10<sup>7</sup> K Hot Emitting Gas in the Circumgalactic Medium of the Milky Way
The Astrophysical Journal · 2024
- A sub-solar Fe/O, log (<i>T</i>/K) ∼ 7.5 gas component permeating the Milky Way’s CGM
Monthly Notices of the Royal Astronomical Society · 2024
- Absorption Studies of the Most Diffuse Gas in the Large-Scale Structure
2024
- Where is the supervirial hot gas? I: a pilot study with sightlines to Galactic X-ray binaries
Monthly Notices of the Royal Astronomical Society · 2024
- arXiv (Cornell University)×25
- Monthly Notices of the Royal Astronomical Society×19
- The Astrophysical Journal×17
- Astronomy and Astrophysics×8
- Research Square×3
- Boyuan Liu
Physics and Astronomy · Purdue University West Lafayette
- Dustin D. Nguyen
Physics and Astronomy · The Ohio State University
- Ying Zu
Physics and Astronomy · The Ohio State University
- J. R. Peterson
Physics and Astronomy · Purdue University West Lafayette
- Debopam Som
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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