A re-analysis of τ U Ma

A re-analysis of the Am star τ U Ma is carried out using new determinations of effective temperature and gravity. The abundances agree in general except a constant factor with those found by Greenstein. The existence of certain heavy elements found in the most cold Ap stars is investigated.

Guardado en:
Detalles Bibliográficos
Autor principal: López-García, Z.
Formato: Articulo Comunicacion
Lenguaje:Inglés
Publicado: 1973
Materias:
Astronomía
Galaxias
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/98707
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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