Temperature Structure and Chemical Abundances in Gaseous Nebulae

2001/06/05 by M. Peimbert, Manuel Peimbert, Peimbert, Manuel
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0106063

5 pages, will appear in the Conference Series of the Revista Mexicana de Astronomia y Astrofisica

arxiv created 2001/06/05 · openalex publication_date 2001/06/05 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

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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