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Joint Optical and Infrared Observations of Nitrogen and Oxygen Reveal the Dust-obscured Gas in Haro 3

Accurate chemical compositions of star-forming regions provide a critical diagnostic tool for characterizing the star formation history and gas flows that regulate galaxy formation. However, the abundance discrepancy factor (ADF) between measurements derived from the “direct” optical electron temper...

Deskribapen osoa

Gorde:
Egile Nagusiak: Yuguang Chen, Tucker Jones, Ryan L. Sanders, Dario Fadda, Jessica Sutter, Robert Minchin, Nikolaus Z. Prusinski, Sunny Rhoades, Keerthi Vasan GC, Charles C. Steidel, Erin Huntzinger, Paige Kelly, Danielle A. Berg, Fabio Bresolin, Rodrigo Herrera-Camus, Ryan J. Rickards Vaught, Guido Roberts-Borsani, Peter Senchyna, Justin S. Spilker, Daniel P. Stark, Benjamin Weiner, D. Christopher Martin, Mateusz Matuszewski, Rosalie C. McGurk, James D. Neill
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: IOP Publishing 2026-01-01
Saila:The Astrophysical Journal
Gaiak:
Chemical abundances
Galaxy evolution
H II regions
Interstellar medium
Sarrera elektronikoa:https://doi.org/10.3847/1538-4357/ae473e
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