Laura A. Lopez
Physics and Astronomy · The Ohio State University
Publications
176
Citations
3,052
Est. group size
~8
Recurring co-author estimate
Active years
54
Publishing since 1973
Laura A. Lopez studies high-energy astrophysics, using X-ray observations to understand how stars, supernovae, and active galactic nuclei inject energy and hot gas into their surroundings. Her work spans supernova remnants (the leftover debris from exploded stars), stellar feedback in star-forming regions, and outflows driven by black holes in galaxy centers, and she is involved in planning future X-ray telescope missions like AXIS. Prospective students would likely work with X-ray data analysis and multi-wavelength observations of galactic and extragalactic gas structures.
Publication output has grown substantially over the last decade, rising from about 4-5 papers per year in 2017-2020 to a peak of 25 in 2023, with continued high output (13-16 per year) in 2024-2025.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- The Spatially Resolved Hot Gas Properties of NGC 1266’s Active Galactic Nucleus-driven Outflow
The Astrophysical Journal · 2026
- The Advanced X-ray Imaging Satellite (AXIS) Community Science Book
arXiv (Cornell University) · 2025
- The Spatially Resolved Hot Gas Properties of NGC 1266's AGN-Driven Outflow
arXiv (Cornell University) · 2025
- Taming the Tarantula: How Stellar Wind Feedback Shapes Gas and Dust in 30 Doradus
arXiv (Cornell University) · 2025
- The Evolution of Galaxies and Clusters at High Spatial Resolution with Advanced X-ray Imaging Satellite (AXIS)
Universe · 2024
- Probing the soft X-ray properties and multi-wavelength variability of SN2023ixf and its progenitor
Publications of the Astronomical Society of Australia · 2024
- Detection of Diffuse Hot Gas around the Young, Potential Superstar Cluster H72.97–69.39
The Astrophysical Journal · 2024
- The Advanced X-ray Imaging Satellite (AXIS)
2024
- Detection of Diffuse Hot Gas Around the Young, Potential Superstar Cluster H72.97-69.39
arXiv (Cornell University) · 2024
- OBSTRUCCION ESOFAGICA SECUNDARIA A BEZOAR DE NUTRICION ENTERAL
2024
- Estimating Ejecta Mass Ratios in Kepler’s Supernova Remnant: Global X-Ray Spectral Analysis Including Suzaku Systematics and Emitting Volume Uncertainties
The Astrophysical Journal · 2023
- Overview of the advanced x-ray imaging satellite (AXIS)
2023
- Probing the Soft X-ray Properties and Multi-Wavelength Variability of SN2023ixf and its Progenitor
arXiv (Cornell University) · 2023
- The evolution of galaxies and clusters at high spatial resolution with AXIS
arXiv (Cornell University) · 2023
- Estimating Ejecta Mass Ratios in Kepler's SNR: Global X-Ray Spectral Analysis Including Suzaku Systematics and Emitting Volume Uncertainties
arXiv (Cornell University) · 2023
- arXiv (Cornell University)×43
- The Astrophysical Journal×17
- The Astrophysical Journal Letters×10
- Monthly Notices of the Royal Astronomical Society×5
- Astronomy and Astrophysics×4
- Kathryn E. Weil
Physics and Astronomy · Purdue University West Lafayette
- Todd A. Thompson
Physics and Astronomy · The Ohio State University
- P. Vallely
Physics and Astronomy · The Ohio State University
- D. Milisavljević
Physics and Astronomy · Purdue University West Lafayette
- Danny Milisavljevic
Physics and Astronomy · Purdue University West Lafayette
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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