Elemental abundances of intermediate-age open cluster NGC 3680

A. W. Mitschang*, G. M. De Silva, D. B. Zucker

*Corresponding author for this work

Research output: Contribution to journalArticle

6 Citations (Scopus)

Abstract

We present a new abundance analysis of the intermediate-age Galactic open cluster NGC 3680, based on high-resolution, high signal-to-noise ratio VLT/UVES spectroscopic data. Several element abundances are presented for this cluster for the first time, but most notably we derive abundances for the light and heavy s-process elements Y, Ba, La and Nd. The serendipitous measurement of the rare-earth r-process element Gd is also reported. This cluster exhibits a significant enhancement of Na in giants as compared to dwarfs, which may be a proxy for an O to Na anticorrelation as observed in Galactic globular clusters but not open clusters. We also observe a step-like enhancement of heavy s-process elements towards higher atomic number, contrary to expectations from asymptotic giant branch nucleosynthesis models, suggesting that the r process played a significant role in the generation of both La and Nd in this cluster.

Original languageEnglish
Pages (from-to)3527-3534
Number of pages8
JournalMonthly Notices of the Royal Astronomical Society
Volume422
Issue number4
DOIs
Publication statusPublished - Jun 2012

Fingerprint Dive into the research topics of 'Elemental abundances of intermediate-age open cluster NGC 3680'. Together they form a unique fingerprint.

Cite this