The VISCACHA survey. VI : dimensional study of the structure of 82 star clusters in the Magellanic Clouds
we present a study of the internal structure of 82 star clusters located at the outer regions of the large magellanic cloud and the small magellanic cloud using data of the Viscacha Survey. Through the construction of the minimum spanning tree, which analyzes the relative position of stars within a...
| Autores: | , , , , , , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2023 |
| País: | Argentina |
| Institución: | Consejo Nacional de Investigaciones Científicas y Técnicas |
| Repositorio: | CONICET Digital (CONICET) |
| Idioma: | inglés |
| OAI Identifier: | oai:ri.conicet.gov.ar:11336/234305 |
| Acceso en línea: | http://hdl.handle.net/11336/234305 |
| Access Level: | acceso abierto |
| Palabra clave: | Magellanic Clouds galaxies: star clusters: general https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| Sumario: | we present a study of the internal structure of 82 star clusters located at the outer regions of the large magellanic cloud and the small magellanic cloud using data of the Viscacha Survey. Through the construction of the minimum spanning tree, which analyzes the relative position of stars within a given cluster, it was possible to characterize the internal structure and explore the fractal or subclustered distribution for each cluster. We computed the parameters (which is the average length of the connectedsegments normalized by the area), (which is the mean points separation in units of cluster radius), and (the ratio of thesecomponents). These parameters are useful to distinguish between radial, homogeneous, and substructured distributions of stars.The dependence of these parameters with the different characteristics of the clusters, such as their ages and spatial distribution,was also studied. We found that most of the studied clusters present a homogeneous stellar distribution or a distribution witha radial concentration. Our results are consistent with the models, suggesting that more dynamically evolved clusters seem tohave larger values, confirming previous results from numerical simulations. There also seems to be a correlation betweenthe internal structure of the clusters and their galactocentric distances, in the sense that for both galaxies, the more distant clusters have larger values. We also paid particular attention to the effects of contamination by non-member field stars and its consequences finding that field star decontamination is crucial for these kinds of studies. |
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