Oxygen and helium abundances in galactic h II regions: abundance gradients

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Main Author: R. Costero
Format: Artículo científico
Language:en
Published: Universidad Nacional Autónoma de México 2000
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author R. Costero
author_facet R. Costero
contents Oxygen and helium abundances in galactic h II regions: abundance gradients R. Costero M. Peña L. Deharveng Física, Astronomía y Matemáticas H II REGIONS ISM: ABUNDANCES GALAXY: ABUNDANCES Absolute integrated uxes have been obtained for 34 H II regions, with Galactocentricdistances RG in the 6.6{17.7 kpc range, in the emission lines [O II] 3726and 3729, [O III] 4363 and 5007, He I 5876, H and H. These uxes are analyzedto derive the physical parameters, the ionic abundances O+/H+, O++/H+and He+/H+ and the O/H abundances. Accurate electron temperatures have beenderived in six H II regions with RG between 6.6 kpc and 14.8 kpc, widening theRG range for which reliable Te measurements exist. Our O/H relationship for5 kpc < RG < 15 kpc is 12 + logO=H = ( 2000 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57100945 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_57100945
institution Redalyc
language en
publishDate 2000
publisher Universidad Nacional Autónoma de México
spellingShingle Oxygen and helium abundances in galactic h II regions: abundance gradients
R. Costero
Física, Astronomía y Matemáticas
H II REGIONS
ISM: ABUNDANCES
GALAXY: ABUNDANCES
Oxygen and helium abundances in galactic h II regions: abundance gradients R. Costero M. Peña L. Deharveng Física, Astronomía y Matemáticas H II REGIONS ISM: ABUNDANCES GALAXY: ABUNDANCES Absolute integrated uxes have been obtained for 34 H II regions, with Galactocentricdistances RG in the 6.6{17.7 kpc range, in the emission lines [O II] 3726and 3729, [O III] 4363 and 5007, He I 5876, H and H. These uxes are analyzedto derive the physical parameters, the ionic abundances O+/H+, O++/H+and He+/H+ and the O/H abundances. Accurate electron temperatures have beenderived in six H II regions with RG between 6.6 kpc and 14.8 kpc, widening theRG range for which reliable Te measurements exist. Our O/H relationship for5 kpc < RG < 15 kpc is 12 + logO=H = ( 2000 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57100945 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 Oxygen and helium abundances in galactic h II regions: abundance gradients
topic Física, Astronomía y Matemáticas
H II REGIONS
ISM: ABUNDANCES
GALAXY: ABUNDANCES
url https://www.redalyc.org/articulo.oa?id=57100945