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Temperature Structure and Chemical Abundances in Gaseous Nebulae
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In this summary I review some results relative to: planetary nebulae, H II regions, chemical evolution of galaxies, and the determination of the primordial helium abundance. These results were presented during the symposium "Ionized Gaseous Nebulae" which took place in Mexico City, Nov, 2000. To get a more general perspective of this meeting I encourage you to read all the contributions to the symposium proceedings.
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Early Results from GLASS-JWST. XXV. Electron Density in the Interstellar Medium at $0.7\lesssim z\lesssim 9.3$ with NIRSpec High-resolution Spectroscopy
JWST high-resolution spectra of 34 lensed galaxies show no significant ISM electron-density evolution between z≈1 and z≈9, plus large scatter between [OII]- and [SII]-derived densities.
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