Nickolas M. Pingel
Physics and Astronomy · Indiana University
Publications
81
Citations
658
Est. group size
—
Recurring co-author estimate
Active years
57
Publishing since 1970
Nickolas M. Pingel studies the gas between stars in our own Milky Way and in nearby galaxies, focusing especially on neutral hydrogen (HI), the raw material from which stars eventually form. Using large radio telescope surveys, this research maps cold atomic gas, its motions and turbulence, and how galaxies interact with their surroundings. Recent work spans the Magellanic Clouds, Local Group dwarf galaxies, and multi-wavelength combinations of radio, optical, and infrared observations.
Publication activity has grown over the last decade, rising from a few papers per year in the late 2010s to roughly nine to eleven per year in recent years.
Generated by claude-opus-4-8 from public bibliographic data · Jul 9, 2026
Typically publishes in teams of ~17 · 12% small-team papers (≤3 authors) · across 19 venues
- The GASKAP-HI Survey towards the Magellanic Clouds: Cold Atomic Gas Survival and Evolution in the Large Magellanic Cloud
arXiv (Cornell University) · 2026
- Diffuse HI emission in the circumgalactic medium of NGC891 and NGC4565 - III: azimuthal profiles
arXiv (Cornell University) · 2026
- Where Do Stars Explode in the ISM?—The Distribution of Dense Gas around Evolved Massive Stars in M33
The Astrophysical Journal · 2026
- The Local Group L -band Survey: Probing Cold Atomic Gas in IC 10 with Neutral Hydrogen Absorption
The Astrophysical Journal · 2026
- Revealing the cold skeleton of the Magellanic Clouds and the Magellanic Bridge with ASKAP
arXiv (Cornell University) · 2026
- Revealing the cold skeleton of the Magellanic clouds and the Magellanic Bridge with ASKAP
Monthly Notices of the Royal Astronomical Society · 2026
- Revisiting Ram Pressure Stripping in Wolf–Lundmark–Melotte: No Evidence for Stripped H I with Local Group L -Band Survey
The Astronomical Journal · 2026
- Revisiting ram pressure stripping in Wolf-Lundmark-Melotte: No evidence for stripped HI with LGLBS
arXiv (Cornell University) · 2026
- The Multi-phase HI of the Milky Way and Nearby Galaxies
arXiv (Cornell University) · 2026
- The Multi-phase HI of the Milky Way and Nearby Galaxies
arXiv (Cornell University) · 2026
- GASKAP pilot survey science. II. 21cm abs.
Strasbourg Astronomical Data Center · 2026
- Relationships between PAHs, Small Dust Grains, H$_2$, and HI in Local Group Dwarf Galaxies NGC 6822 and WLM Using JWST, ALMA, and the VLA
arXiv (Cornell University) · 2025
- Relationships between Polycyclic Aromatic Hydrocarbons, Small Dust Grains, H2, and H i in Local Group Dwarf Galaxies NGC 6822 and WLM Using JWST, ALMA, and the VLA
The Astrophysical Journal · 2025
- Study of HI Turbulence in the SMC Using Multi-point Structure Functions
arXiv (Cornell University) · 2025
- The Local Group L-band Survey: Probing Cold Atomic Gas in IC10 with Neutral Hydrogen Absorption
arXiv (Cornell University) · 2025
- arXiv (Cornell University)×19
- The Astrophysical Journal×12
- Monthly Notices of the Royal Astronomical Society×12
- The Astronomical Journal×3
- Publications of the Astronomical Society of Australia×2
- Molly Gallagher
Physics and Astronomy · The Ohio State University
- Adam K. Leroy
Physics and Astronomy · The Ohio State University
- Dyas Utomo
Physics and Astronomy · The Ohio State University
- Jiayi Sun
Physics and Astronomy · The Ohio State University
- William J. Gray
Physics and Astronomy · University of Michigan
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Sep 1, 2026.
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