AggieSTAAR: Introduction to HII Regions
Jun 20, 2025·
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0 min read
Ray Garner
The War & Peace Nebula, NGC 6357. Credit: Guillermo (Guy) YanezAbstract
This talk was given as part of a weekly lunch talk for the undergraduate researchers in the Aggie Scholarships for Technology Advancements in Astronomical Research (AggieSTAAR) program. In this talk, I gave an overview of H II regions, what they are and how we use atomic physics to study them. I talked in detail about photoionization and recombination and how metals are necessary to cool H II regions. After giving an example spectrum, I introduced how we measure the oxygen abundance of H II regions via the direct method as well as strong-line methods. Finally, I used my experience in the SIGNALS collaboration to show some applications of what we learn about galaxies after estimating H II region abundances. The talk was followed by a Q&A session with the undergraduates, ranging from research to job prospects.
Date
Jun 20, 2025 12:00 PM — 1:30 PM
Location
Texas A&M University - Munnerlyn Astronomy & Space Sciences Engineering Building
4242 TAMU, College Station, Texas 77843

Authors
Ray Garner
(he/him)
TAMU Astronomy Postdoctoral Researcher
I’m a scientist, Star Wars fan, and amateur photographer raised in Georgia. My research interests include galaxy evolution, star formation, and nebular diagnostics.