Stellar populations in dwarf elliptical galaxies: a photometrical approach

Several constraints upon stellar populations in dwarf elliptical (dE) galaxies are derived from integrated Washington colors of a sample of 12 Fornax cluster dE's. To do so, the dE's colors are compared to observed colors of Galactic globular clusters and synthetic colors integrated from s...

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Autores principales: Cellone, Sergio Aldo, Forte, Juan Carlos
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1994
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/159858
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spelling I19-R120-10915-1598582023-11-07T20:01:46Z http://sedici.unlp.edu.ar/handle/10915/159858 Stellar populations in dwarf elliptical galaxies: a photometrical approach Cellone, Sergio Aldo Forte, Juan Carlos 1994 2023-11-07T11:31:30Z es Astronomía Galaxia Several constraints upon stellar populations in dwarf elliptical (dE) galaxies are derived from integrated Washington colors of a sample of 12 Fornax cluster dE's. To do so, the dE's colors are compared to observed colors of Galactic globular clusters and synthetic colors integrated from spectral energy distributions, both observed and theoretical, simple stellar populations. The position of the dwarfs in a color - color plot (C — T) vs M — Tᵢ) suggests metallicities comparable to those of moderately rich globular. However, some galaxies depart from the sequence defined by the globulars; their color can only be reproduced by a mix of an old, moderately rich dominant population, plus contribution from a younger population (∼ 5 x 10⁸ yr). The fact that one galaxy with independent evidences for a recent star formation event lies at the blue end of this sequence, strongly supports our conclusion. Asociación Argentina de Astronomía Articulo Comunicacion http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxia
spellingShingle Astronomía
Galaxia
Cellone, Sergio Aldo
Forte, Juan Carlos
Stellar populations in dwarf elliptical galaxies: a photometrical approach
topic_facet Astronomía
Galaxia
description Several constraints upon stellar populations in dwarf elliptical (dE) galaxies are derived from integrated Washington colors of a sample of 12 Fornax cluster dE's. To do so, the dE's colors are compared to observed colors of Galactic globular clusters and synthetic colors integrated from spectral energy distributions, both observed and theoretical, simple stellar populations. The position of the dwarfs in a color - color plot (C — T) vs M — Tᵢ) suggests metallicities comparable to those of moderately rich globular. However, some galaxies depart from the sequence defined by the globulars; their color can only be reproduced by a mix of an old, moderately rich dominant population, plus contribution from a younger population (∼ 5 x 10⁸ yr). The fact that one galaxy with independent evidences for a recent star formation event lies at the blue end of this sequence, strongly supports our conclusion.
format Articulo
Comunicacion
author Cellone, Sergio Aldo
Forte, Juan Carlos
author_facet Cellone, Sergio Aldo
Forte, Juan Carlos
author_sort Cellone, Sergio Aldo
title Stellar populations in dwarf elliptical galaxies: a photometrical approach
title_short Stellar populations in dwarf elliptical galaxies: a photometrical approach
title_full Stellar populations in dwarf elliptical galaxies: a photometrical approach
title_fullStr Stellar populations in dwarf elliptical galaxies: a photometrical approach
title_full_unstemmed Stellar populations in dwarf elliptical galaxies: a photometrical approach
title_sort stellar populations in dwarf elliptical galaxies: a photometrical approach
publishDate 1994
url http://sedici.unlp.edu.ar/handle/10915/159858
work_keys_str_mv AT cellonesergioaldo stellarpopulationsindwarfellipticalgalaxiesaphotometricalapproach
AT fortejuancarlos stellarpopulationsindwarfellipticalgalaxiesaphotometricalapproach
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