Astrophysical properties of star clusters in the Magellanic Clouds homogeneously estimated by ASteCA

Aims. To produce an homogeneous catalog of astrophysical parameters of 239 resolved star clusters located in the Small and Large Magellanic Clouds, observed in the Washington photometric system. Methods. The cluster sample was processed with the recently introduced Automated Stellar Cluster Analysi...

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Autores principales: Perren, Gabriel Ignacio, Piatti, Andrés, Vázquez, Rubén Ángel
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2017
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/82208
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id I19-R120-10915-82208
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
catalogs
galaxies: fundamental parameters
galaxies: star clusters: general
Magellanic Clouds
methods: statistical
techniques: photometric
spellingShingle Ciencias Astronómicas
catalogs
galaxies: fundamental parameters
galaxies: star clusters: general
Magellanic Clouds
methods: statistical
techniques: photometric
Perren, Gabriel Ignacio
Piatti, Andrés
Vázquez, Rubén Ángel
Astrophysical properties of star clusters in the Magellanic Clouds homogeneously estimated by ASteCA
topic_facet Ciencias Astronómicas
catalogs
galaxies: fundamental parameters
galaxies: star clusters: general
Magellanic Clouds
methods: statistical
techniques: photometric
description Aims. To produce an homogeneous catalog of astrophysical parameters of 239 resolved star clusters located in the Small and Large Magellanic Clouds, observed in the Washington photometric system. Methods. The cluster sample was processed with the recently introduced Automated Stellar Cluster Analysis (ASteCA) package, which ensures both an automatized and a fully reproducible treatment, together with a statistically based analysis of their fundamental parameters and associated uncertainties. The fundamental parameters determined with this tool for each cluster, via a color-magnitude diagram (CMD) analysis, are: metallicity, age, reddening, distance modulus, and total mass. Results. We generated an homogeneous catalog of structural and fundamental parameters for the studied cluster sample, and performed a detailed internal error analysis along with a thorough comparison with values taken from twenty-six published articles. We studied the distribution of cluster fundamental parameters in both Clouds, and obtained their age-metallicity relationships. Conclusions. The ASteCA package can be applied to an unsupervised determination of fundamental cluster parameters; a task of increasing relevance as more data becomes available through upcoming surveys.
format Articulo
Preprint
author Perren, Gabriel Ignacio
Piatti, Andrés
Vázquez, Rubén Ángel
author_facet Perren, Gabriel Ignacio
Piatti, Andrés
Vázquez, Rubén Ángel
author_sort Perren, Gabriel Ignacio
title Astrophysical properties of star clusters in the Magellanic Clouds homogeneously estimated by ASteCA
title_short Astrophysical properties of star clusters in the Magellanic Clouds homogeneously estimated by ASteCA
title_full Astrophysical properties of star clusters in the Magellanic Clouds homogeneously estimated by ASteCA
title_fullStr Astrophysical properties of star clusters in the Magellanic Clouds homogeneously estimated by ASteCA
title_full_unstemmed Astrophysical properties of star clusters in the Magellanic Clouds homogeneously estimated by ASteCA
title_sort astrophysical properties of star clusters in the magellanic clouds homogeneously estimated by asteca
publishDate 2017
url http://sedici.unlp.edu.ar/handle/10915/82208
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