Subir material

Suba sus trabajos a SEDICI, para mejorar notoriamente su visibilidad e impacto

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2022-10-31T12:14:33Z
dc.date.available 2022-10-31T12:14:33Z
dc.date.issued 1992
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/144795
dc.description.abstract New empirical DDO abundance calibrations for population I and II late-type giants are presented. Blanketing vectors and isoabundance lines in the EDO two-color diagrams are determined. The new abundance index, δ4548, correlates very well with the metallicity even for stars with [Fe/H] = -3.0. New DDO abundance determinations in open and globular cluster giants show general good agreement with the scales of Friel and Janes (1992, A&A, in press) and Zinn (1985, Ap.J. 293, 424), for open and globular clusters, respectively. This paper will be published in detail elsewhere. en
dc.language es es
dc.subject Galaxia es
dc.title Metallicities of open and globular cluster giants determined from new DDO abundance calibrations en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Clariá, J.J. es
sedici.creator.person Minniti, D. es
sedici.creator.person Piatti, A. es
sedici.creator.person Lappaset, E. es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 37 es
dc.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/ es
dc.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)


Descargar archivos

Thumbnail
Resumen (3 p.)
Descargar archivo (289.9Kb) - PDF

Este ítem aparece en la(s) siguiente(s) colección(ones)

Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)