On the line shift and oscillator strength of Xe II lines in the spectra of HnMn stars

Aims. The ultimate goal that has motivated this work is to achieve realistic oscillator strength (<i>gf</i>) values to find reliable values of stellar abundances. We aim to compare the <i>gf</i> valúes of Xe ii lines found with different theoretical and experimental methods....

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Detalles Bibliográficos
Autores principales:	Di Rocco, Héctor O., Cruzado, Alicia, Marchiano, Paula Esther
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2015
Materias:	Ciencias Astronómicas Atomic data Line: identification Stars: abundances Stars: chemically peculiar
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/86392
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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