RMxAA

Revista Mexicana de Astronomía y Astrofísica

ISSN: 3061-8649
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Keywords

Distance
Planetary Nebulae
Interstellar Matter
Stellar Mass
Hertzsprung-Russell Diagram
Astrophysics
Planetary Nebulae: Distances
Planetary Nebulae: Central Stars
Planetary Nebulae: Metal Abundances
Central Stars: Masses

How to Cite

Distances of Galactic Planetary Nebulae Based on a Relationship Between the Central Star Mass and the N/O Abundance. (2000). Revista Mexicana De Astronomía Y Astrofísica, 36(1), 3. https://astronomia.unam.mx/journals/rmxaa/article/view/2000rmxaa..36....3c

Abstract

The author propose a method to determine distances of Galactic planetary nebulae on the basis of a relationship between the central star mass Mc and the nebular N/O abundance ratio. This relationship is used in combination with some basic parameters of the central stars, such as the λ5480 Å flux, surface gravity and visual magnitude in order to obtain distances to a sample of a hundred Galactic planetary nebulae.
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