SIMBAD references

2007AJ....134..391C - Astron. J., 134, 391-410 (2007/July-0)

Stellar populations of globular clusters in the elliptical galaxy NGC 1407.

CENARRO A.J., BEASLEY M.A., STRADER J., BRODIE J.P. and FORBES D.A.

Abstract (from CDS):

We present high-quality Keck spectroscopic data for a sample of 20 globular clusters (GCs) in the massive E0 galaxy NGC 1407. A subset of 20 line-strength indices of the Lick/IDS system has been measured for both the GC system and the central integrated starlight of the galaxy. Ages, metallicities, and [α/Fe] ratios have been derived using several different approaches. The majority of GCs in NGC 1407 studied are old, follow a tight metallicity sequence reaching values slightly above solar, and exhibit mean [α/Fe] ratios of ∼0.3 dex. In addition, three GCs are formally derived to be young (∼4 Gyr), but we argue that they are actually old GCs hosting blue horizontal branches. We report, for the first time, evidence for the existence of two chemically distinct subpopulations of metal-rich (MR) GCs. We find that some MR GCs exhibit significantly larger [Mg/Fe] and [C/Fe] ratios. Different star formation timescales are proposed to explain the correlation between Mg and C abundances. We also find striking CN overabundances over the entire GC metallicity range. It is interesting to note that the behavior of C and N in metal-poor GCs clearly deviates from that in MR GCs. In particular, for MR GCs, N increases dramatically while C essentially saturates. This may be interpreted as a consequence of the increasing importance of the CNO cycle with increasing metallicity.

Abstract Copyright:

Journal keyword(s): Galaxies: Clusters: General - Galaxies: Formation - Galaxies: Star Clusters - Galaxy: Globular Clusters: General

Nomenclature: Table 1: [CBS2007] NN N=21 among (Nos 1-33).

Simbad objects: 52

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2007AJ....134..391C and select 'bookmark this link' or equivalent in the popup menu


2019.10.14-08:53:18

© Université de Strasbourg/CNRS

    • Contact