AGE-METALLICITY DEGENERACY AT MID-UV WAVELENGTHS

Fuente: Redalyc
Saved in:
Bibliographic Details
Main Author: E. Bertone
Format: Artículo científico
Language:en
Published: Universidad Nacional Autónoma de México 2009
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1876433303572054016
author E. Bertone
author_facet E. Bertone
contents AGE-METALLICITY DEGENERACY AT MID-UV WAVELENGTHS E. Bertone M. Chavez A. Buzzoni Física, Astronomía y Matemáticas ultraviolet: galaxies galaxies: stellar content Galaxies: fundamental parameters The so-called age-metallicity degeneracy, which a ects the optical spectral properties of stellar populations, is also present at mid-ultraviolet wavelengths. We give here the results for two reference objects: the Sun (assumed as representative of the turno star of a single stellar population) and M32. Within a theoretical framework, we have explored the properties of the age-metallicity degeneracy by means of 17 spectroscopic indices from 2100 to 3100 A: our preliminary results show a metallicity sensitivity parameter value of 1.7=1.2, which is compatible with the Worthey's value of 3/2 in the optical interval. 2009 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57115687021 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.37
format Artículo científico
id redalyc_57115687021
institution Redalyc
language en
publishDate 2009
publisher Universidad Nacional Autónoma de México
spellingShingle AGE-METALLICITY DEGENERACY AT MID-UV WAVELENGTHS
E. Bertone
Física, Astronomía y Matemáticas
ultraviolet: galaxies
galaxies: stellar content
Galaxies: fundamental parameters
AGE-METALLICITY DEGENERACY AT MID-UV WAVELENGTHS E. Bertone M. Chavez A. Buzzoni Física, Astronomía y Matemáticas ultraviolet: galaxies galaxies: stellar content Galaxies: fundamental parameters The so-called age-metallicity degeneracy, which a ects the optical spectral properties of stellar populations, is also present at mid-ultraviolet wavelengths. We give here the results for two reference objects: the Sun (assumed as representative of the turno star of a single stellar population) and M32. Within a theoretical framework, we have explored the properties of the age-metallicity degeneracy by means of 17 spectroscopic indices from 2100 to 3100 A: our preliminary results show a metallicity sensitivity parameter value of 1.7=1.2, which is compatible with the Worthey's value of 3/2 in the optical interval. 2009 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57115687021 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.37
title AGE-METALLICITY DEGENERACY AT MID-UV WAVELENGTHS
topic Física, Astronomía y Matemáticas
ultraviolet: galaxies
galaxies: stellar content
Galaxies: fundamental parameters
url https://www.redalyc.org/articulo.oa?id=57115687021