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The Astrophysical Journal
Article . 1984 . Peer-reviewed
Data sources: Crossref
https://dx.doi.org/10.1086/162...
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Metal abundances of galactic globular clusters

descriptionPublicationkeyboard_double_arrow_right Article 01 Jun 1984 English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 281, page 148 (issn: 0004-637X, eissn: 1538-4357, Copyright policy )
Authors: H. A. Smith;

doi: 10.1086/162084

Metal abundances of galactic globular clusters

Abstract

On a mesure l'indice ΔS de l'abondance en metaux pour les etoiles RR Lyrae de neuf amas globulaires. Il y a une bonne correlation entre ΔS et l'indice de temperature de la branche des geantes (V-K) 0 GB. Les abondances ΔS de 26 amas globulaires ont ete utilisees pour re-etalonner l'indice de Zinn Q 39 en fonction de [Fe/H]. On a determine les valeurs de [Fe/H] pour 55 amas globulaires, soit a partir de ΔS, soit a partir des indices Q 39 corriges

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
12
Average
Average
Average
gold