O2+ Recombination abundances in planetary nebulae

Fuente: Redalyc
Saved in:
Bibliographic Details
Main Author: R. L. Kingsburgh
Format: Artículo científico
Language:en
Published: Universidad Nacional Autónoma de México 2001
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1876472909583613952
author R. L. Kingsburgh
author_facet R. L. Kingsburgh
contents O2+ Recombination abundances in planetary nebulae R. L. Kingsburgh M. H. Armour Física, Astronomía y Matemáticas ERAL ISM: ABUNDANCES PLANETARY NEBULAE: GEN We present O2+/H+ abundances derived from echelle spectroscopy of fourplanetary nebulae, NGC 6210, NGC 6826, Hu2{1, NGC 6543, from the forbidden,collisionally excited lines, and from the permitted recombination lines. We ndthat the ratio of the recombination line to collisional line abundances ranges fromessentially unity (1.2 for Hu 2{1) to 6.6, for an o set position of NGC 6826, andcorresponding t2 values range from 0.016 to 0.087. 2001 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101013 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.10
format Artículo científico
id redalyc_57101013
institution Redalyc
language en
publishDate 2001
publisher Universidad Nacional Autónoma de México
spellingShingle O2+ Recombination abundances in planetary nebulae
R. L. Kingsburgh
Física, Astronomía y Matemáticas
ERAL
ISM: ABUNDANCES
PLANETARY NEBULAE: GEN
O2+ Recombination abundances in planetary nebulae R. L. Kingsburgh M. H. Armour Física, Astronomía y Matemáticas ERAL ISM: ABUNDANCES PLANETARY NEBULAE: GEN We present O2+/H+ abundances derived from echelle spectroscopy of fourplanetary nebulae, NGC 6210, NGC 6826, Hu2{1, NGC 6543, from the forbidden,collisionally excited lines, and from the permitted recombination lines. We ndthat the ratio of the recombination line to collisional line abundances ranges fromessentially unity (1.2 for Hu 2{1) to 6.6, for an o set position of NGC 6826, andcorresponding t2 values range from 0.016 to 0.087. 2001 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101013 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.10
title O2+ Recombination abundances in planetary nebulae
topic Física, Astronomía y Matemáticas
ERAL
ISM: ABUNDANCES
PLANETARY NEBULAE: GEN
url https://www.redalyc.org/articulo.oa?id=57101013