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...
Guardado en:
| Autores principales: | , , |
|---|---|
| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2017
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/82208 |
| Aporte de: |
| 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 |
| work_keys_str_mv |
AT perrengabrielignacio astrophysicalpropertiesofstarclustersinthemagellaniccloudshomogeneouslyestimatedbyasteca AT piattiandres astrophysicalpropertiesofstarclustersinthemagellaniccloudshomogeneouslyestimatedbyasteca AT vazquezrubenangel astrophysicalpropertiesofstarclustersinthemagellaniccloudshomogeneouslyestimatedbyasteca |
| bdutipo_str |
Repositorios |
| _version_ |
1764820487999848448 |