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Keywords

early universe
galaxies: abundances
H II regions
ISM: abundances
planetary nebulae
Astrophysics

How to Cite

Temperature Structure and Chemical Abundances in Gaseous Nebulae. (2002). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 12(1), 275-279. https://astronomia.unam.mx/journals/rmxac/article/view/2002rmxac..12..275p
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Abstract

In this summary I review some of the results presented in this symposium relating to planetary nebulae, H II regions, chemical evolution of galaxies, and the determination of the primordial helium abundance. To get a more general perspective of this symposium I encourage you to read all the contributions to these proceedings.