Artículo
Observational hints of a real age spread in the young LMC star cluster NGC 1971
Fecha de publicación:
09/2017
Editorial:
Wiley Blackwell Publishing, Inc
Revista:
Monthly Notices of the Royal Astronomical Society: Letters
ISSN:
1745-3933
Idioma:
Inglés
Tipo de recurso:
Artículo publicado
Clasificación temática:
Resumen
We report that the serendipitous young Large Magellanic Cloud cluster NGC 1971 exhibits an extended main-sequence turn-off (eMSTO) possibly originated mostly by a real age spread. We used CT1 Washington photometry to produce a colour–magnitude diagram (CMD) with the fiducial cluster features. From its eMSTO, we estimated an age spread of ∼170 Myr (observed age range 100–280 Myr), once observational errors, stellar binarity, overall metallicity variations and stellar rotation effects were subtracted in quadrature from the observed age width.
Palabras clave:
Cluster
Archivos asociados
Licencia
Identificadores
Colecciones
Articulos(CCT - CORDOBA)
Articulos de CTRO.CIENTIFICO TECNOL.CONICET - CORDOBA
Articulos de CTRO.CIENTIFICO TECNOL.CONICET - CORDOBA
Citación
Piatti, Andres Eduardo; Cole, Andrew; Observational hints of a real age spread in the young LMC star cluster NGC 1971; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society: Letters; 470; 1; 9-2017; L77-L81
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