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Uncertainties of Synthetic Integrated Colors as Age Indicators
Author(s) -
Sukyoung K. Yi
Publication year - 2003
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/344640
Subject(s) - metallicity , globular cluster , galaxy , stellar population , redshift , astrophysics , stars , degeneracy (biology) , physics , astronomy , star formation , bioinformatics , biology
We investigate the uncertainties in the synthetic integrated colors of simplestellar populations. Three types of uncertainties are from the stellar models,the population synthesis techniques, and from the spectral libraries. Despitesome skepticism, synthetic colors appear to be reliable age indicators whenused for select age ranges. Rest-frame optical colors are good age indicatorsat ages 2 -- 7Gyr. At ages sufficiently large to produce hot HB stars, theUV-to-optical colors provide an alternative means for measuring ages. This UVtechnique may break the age-metallicity degeneracy because it separates oldpopulations from young ones even in the lack of metallicity information. Onecan use such techniques on extragalactic globular clusters and perhaps even forhigh redshift galaxies that are passively evolving to study galaxy evolutionhistory.Comment: 38 pages, 21 figures, LaTex, 2003, ApJ, 582 (Jan 1), in pres

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