There is no single density: star-forming regions and galaxies hold more dense ionized gas than long assumed
J. Eduardo Méndez-Delgado, Christophe Morisset, William J. Henney, Niv Drory, Oleg V. Egorov, Sebastián F. Sánchez, Juna A. Kollmeier, Kathryn Kreckel, Guillermo Blanc, Grażyna Stasińska, Evelyn J. Johnston, Héctor J. Ibarra-Medel, Alfredo J. Mejía-Narváez, César Esteban, Jorge García-Rojas, Amrita Singh, Ivan Yu. Katkov, Evan D. Skillman, Rogelio Orozco-Duarte, Igor A. Zinchenko, Alejandra Z. Lugo-Aranda, Aida Wofford, Simon C. O. Glover, Evgeniya Egorova, Rodolfo de J. Zermeño, Lesly C. Castañeda-Carlos, Fu-Heng Liang, Natascha Sattler, Irene Cruz-González, Joel R. Brownstein, Thomas Hilder, Donald P. Schneider
astro-ph.GA
Submitted: 2026-07-08
Comments: Submitted manuscript; comments welcome
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- SDSS-V LVM: Revealing the Physical and Chemical Structure of the Helix Nebula
- The Sunburst Arc with JWST: III. An Abundance of Direct Chemical Abundances
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