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Los cúmulos abiertos son objetos muy útiles en astrofísica; se han utilizado para estudiar la teoría de la formación y la evolución estelar, así como la estructura de la vía láctea. En ese contexto, se analizaron estrellas enanas y gigantes pertenecientes a los cúmulos abiertos IC 2391 y NGC 6475. Los espectros de alta resolución se obtuvieron de la base de datos ESO/Archive. Para obtener los parámetros atmosféricos (Teff, log g, ε, [Fe/H]) y las abundancias químicas, se aplicó la hipótesis del equilibrio termodinámico local (local thermodynamic equilibrium, LTE). Nuestros resultados corroboraron el comportamiento de las abundancias químicas en el disco galáctico.
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Derechos de autor 2023 Revista de la Academia Colombiana de Ciencias Exactas, Físicas y Naturales