D. M. Terndrup
Physics and Astronomy · The Ohio State University
Publications
206
Citations
6,559
Est. group size
—
Recurring co-author estimate
Active years
42
Publishing since 1984
D. M. Terndrup's research focuses on quasars, extremely luminous and distant galactic centers powered by supermassive black holes, particularly those showing broad absorption lines caused by fast-moving gas outflows. Much of the work uses spectral-synthesis modeling (SimBAL) to characterize the physical properties, location, and energy of these outflows in a class of objects called FeLoBAL quasars. This research contributes to understanding how quasars eject and shape surrounding gas, which is relevant to galaxy evolution.
Publication output has been fairly steady but modest over the last decade, fluctuating between roughly 2 and 6 papers per year without a clear upward or downward trend.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- Balmer Absorption in Iron Low-ionization Broad Absorption Line Quasars
The Astrophysical Journal · 2025
- Balmer Absorption in Iron Low-Ionization Broad Absorption Line Quasars
arXiv (Cornell University) · 2025
- The Physical Properties of Low-redshift FeLoBAL Quasars. IV. Optical–Near-IR Spectral Energy Distributions and Near-IR Variability Properties
The Astrophysical Journal · 2024
- The Physical Properties of Low Redshift FeLoBAL Quasars. IV. Optical-Near IR Spectral Energy Distributions and Near-IR Variability Properties
arXiv (Cornell University) · 2024
- Investigating the Origin of the Absorption-line Variability in the Narrow-line Seyfert 1 Galaxy WPVS 007
The Astrophysical Journal · 2023
- The Dragonfly Galaxy. III. Jet Brightening of a High-redshift Radio Source Caught in a Violent Merger of Disk Galaxies
The Astrophysical Journal · 2023
- The Dragonfly Galaxy. III. Jet-brightening of a High-redshift Radio Source Caught in a Violent Merger of Disk Galaxies
arXiv (Cornell University) · 2023
- The Physical Properties of Low-redshift FeLoBAL Quasars. I. Spectral-synthesis Analysis of the Broad Absorption-line (BAL) Outflows Using SimBAL
The Astrophysical Journal · 2022
- The Physical Properties of Low-redshift FeLoBAL Quasars. III. The Location and Geometry of the Outflows
The Astrophysical Journal · 2022
- The Physical Properties of Low Redshift FeLoBAL Quasars. I. Spectral Synthesis Analysis of the BAL Outflows using $SimBAL$
arXiv (Cornell University) · 2022
- The Physical Properties of Low-redshift FeLoBAL Quasars. II. The Rest-frame Optical Emission Line Properties
The Astrophysical Journal · 2022
- Exploring the physics and energetics of FeLoBAL outflows
43rd COSPAR Scientific Assembly. Held 28 January - 4 February · 2021
- Characterizing the Properties of Powerful Quasar Outflows with SimBAL
43rd COSPAR Scientific Assembly. Held 28 January - 4 February · 2021
- Discovery of a Remarkably Powerful Broad Absorption-line Quasar Outflow in SDSS J135246.37+423923.5
The Astrophysical Journal · 2020
- The z = 0.54 LoBAL Quasar SDSS J085053.12+445122.5. II. The Nature of Partial Covering in the Broad-absorption-line Outflow
The Astrophysical Journal · 2019
- The Astrophysical Journal×14
- arXiv (Cornell University)×6
- Monthly Notices of the Royal Astronomical Society×3
- AAS×3
- yCat×2
- Enrico Vesperini
Physics and Astronomy · Indiana University
- Alison Duck
Physics and Astronomy · The Ohio State University
- C. A. Pilachowski
Physics and Astronomy · Indiana University
- B. Scott Gaudi
Physics and Astronomy · The Ohio State University
- Constantine P. Deliyannis
Physics and Astronomy · Indiana 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.
Claim or correct this profile