NGC 4337: an over-looked old cluster in the inner disc of the Milky Way

Abstract

Galactic open clusters do not survive long in the high density regions of the inner Galactic disc. Inside the solar ring only 11 open clusters are known with ages older than one Gyr. We show here, basing on deep, high-quality photometry, that NGC 4337, contrary to earlier findings, is indeed an old open cluster. The cluster is located very close to the conspicuous star cluster Trumpler 20, as well mis-classified in the past, and that has received so much attention in recent years. NGC 4337 shows a significant clump of He-burning stars which was not detected previously. Its beautiful color-magnitude diagram is strikingly similar to the one of the classical old open clusters IC 4651, NGC 752, and NGC 3680, and this suggests similar age and composition. A spectroscopic study is much needed to confirm our findings. This, in turn, would also allow us to better define the inner disc radial abundance gradient and its temporal evolution.To this aim, a list of clump star candidates is provided.

5 pages, 4 eps figures, in press as MNRAS Letter

References in corpus (3)

• On the metallicity of open clusters I. Photometry
• Fundamental parameters of six neglected old open clusters
• Trumpler 20 - an old and rich open cluster

Cited by in corpus (6)

• ASteCA - Automated Stellar Cluster Analysis
• A uvbyCaHbeta Analysis of the Old Open Cluster, NGC 6819
• An investigation of poorly studied open cluster NGC 4337 using multi-color photometric and Gaia DR2 astrometric data
• On the mass of the Galactic star cluster NGC 4337
• Abundance analysis of red clump stars in the old, inner disc, open cluster NGC 4337: a twin of NGC 752?
• On the assessment of the nature of open star clusters and the determination of their basic parameters with limited data