A re-analysis of τ U Ma

dc.creatorLópez-García, Z.
dc.date1973
dc.date2020-06-22T13:39:06Z
dc.date.accessioned2023-07-14T21:03:24Z
dc.date.available2023-07-14T21:03:24Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/98707
dc.identifierissn:1669-9521
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7441624
dc.descriptionA 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.
dc.descriptionAsociación Argentina de Astronomía
dc.formatapplication/pdf
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectAstronomía
dc.subjectGalaxias
dc.titleA re-analysis of τ U Ma
dc.typeArticulo
dc.typeComunicacion


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