50 years of temperature inhomogeneities in gaseous nebulae

2019/05/03 by M. Peimbert, Peimbert, Manuel
Engineering · Physics and Astronomy · #Astro and Planetary Science #Astrophysics of Galaxies (astro-ph.GA) #FOS: Physical sciences #Solar and Stellar Astrophysics (astro-ph.SR) #Spacecraft and Cryogenic Technologies #Stellar, planetary, and galactic studies

paper · pdf · doi:10.48550/arxiv.1905.01244

openalex publication_date 2019/05/03 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

A review of some of the papers that discuss the relevance of the temperature structure present in H II regions and planetary nebulae is presented. Particular attention is given to the determination of the chemical abundances of these objects.

Related

• Temperature Structure and Chemical Abundances in Gaseous Nebulae
• 'Chemical abundances in H II regions and their implications -- Retrospective on: M. Peimbert & R. Costero, Boletin de los Observatorios de Tonantzintla y Tacubaya, Vol. 5, 3, 1969'
• The Temperature Structure in Ionized Nebulae and the Chemical Evolution\n of Galaxies
• Temperature Variations and Abundance Determinations in Planetary Nebulae
• The electron temperature in ionized nebulae