New Metallicities of Rr Lyrae Stars in Omega Centauri: Evidence for a Non-He-Enhanced Metal-Intermediate Population

Simple item page
dc.contributor.authorSollima, A.
dc.contributor.authorCatelan, Márcio
dc.contributor.authorMinniti, D.
dc.date.accessioned2017-04-25T19:28:29Z
dc.date.available2017-04-25T19:28:29Z
dc.date.issued2006
dc.identifier.doi10.1086/503099
dc.identifier.issn0004-637X
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/20977
dc.identifier.urihttps://doi.org/10.1086/503099
dc.language.isoen
dc.relation.isformatofAstrophysical Journal Vol. 640, no. 1 (2006), p. [L43]-L46
dc.revistaAstrophysical Journales_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas RR Lyraees_ES
dc.subject.otherEstrellas - Cúmulos globulareses_ES
dc.subject.otherAstronomía - Observacioneses_ES
dc.titleNew Metallicities of Rr Lyrae Stars in Omega Centauri: Evidence for a Non-He-Enhanced Metal-Intermediate Populationes_ES
dc.typeartículo
sipa.codpersvinculados1001556
sipa.codpersvinculados100504
Files
Original bundle
Now showing 1 - 1 of 1
Thumbnail Image
Name:
New Metallicities of Rr Lyrae Stars in Omega Centauri- Evidence for a Non-He-Enhanced Metal-Intermediate Population.pdf
Size:
120.91 KB
Format:
Adobe Portable Document Format
Description:
Download
Collections
Artículos de revistas