Physical parameters and chemical composition in abell 78

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Main Author: Miriam Peña
Format: Artículo científico
Language:en
Published: Universidad Nacional Autónoma de México 2000
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author Miriam Peña
author_facet Miriam Peña
contents Physical parameters and chemical composition in abell 78 Miriam Peña Selene Medina Física, Astronomía y Matemáticas AGB VIDUAL (A 78) ISM: ABUNDANCES STARS: AGB AND POST PLANETARY NEBULAE: INDI Physical parameters and chemical abundances were derived for di erent zonesof A78, from a high resolution spectroscopic study. The zones observed are thebright central knots and the outer hydrogen-rich shell. The knots contain an extremelyhydrogen-decient material and the composition of this zone is dominatedby helium and heavy elements. The hydrogen-rich external shell appears to havenormal helium abundance and very low metallicity. We conclude that the abundancedetermination is a ected by the presence of large temperature uctuations inthe gas, due to additional heating mechanisms such as shocks by high speed ejectaand photoelectrons from dust grains. 2000 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57100960 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.9
format Artículo científico
id redalyc_57100960
institution Redalyc
language en
publishDate 2000
publisher Universidad Nacional Autónoma de México
spellingShingle Physical parameters and chemical composition in abell 78
Miriam Peña
Física, Astronomía y Matemáticas
AGB
VIDUAL (A 78)
ISM: ABUNDANCES
STARS: AGB AND POST
PLANETARY NEBULAE: INDI
Physical parameters and chemical composition in abell 78 Miriam Peña Selene Medina Física, Astronomía y Matemáticas AGB VIDUAL (A 78) ISM: ABUNDANCES STARS: AGB AND POST PLANETARY NEBULAE: INDI Physical parameters and chemical abundances were derived for di erent zonesof A78, from a high resolution spectroscopic study. The zones observed are thebright central knots and the outer hydrogen-rich shell. The knots contain an extremelyhydrogen-decient material and the composition of this zone is dominatedby helium and heavy elements. The hydrogen-rich external shell appears to havenormal helium abundance and very low metallicity. We conclude that the abundancedetermination is a ected by the presence of large temperature uctuations inthe gas, due to additional heating mechanisms such as shocks by high speed ejectaand photoelectrons from dust grains. 2000 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57100960 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.9
title Physical parameters and chemical composition in abell 78
topic Física, Astronomía y Matemáticas
AGB
VIDUAL (A 78)
ISM: ABUNDANCES
STARS: AGB AND POST
PLANETARY NEBULAE: INDI
url https://www.redalyc.org/articulo.oa?id=57100960