High resolution spectroscopic study of red clump stars in the Galaxy: iron group elements

TL;DR

This study provides high-resolution spectroscopic analysis of 62 red clump stars in the Galaxy, revealing their atmospheric parameters and iron group element abundances, supporting models of their age and metallicity distribution.

Contribution

It offers detailed elemental abundances and atmospheric parameters for a homogeneous sample of red clump stars, confirming their near-solar metallicity and young age in the local disk.

Findings

Mean metallicity [Fe/H] = -0.01 dex with small dispersion

Iron group element ratios close to solar

Supports the model of nearby clump stars being relatively young

Abstract

The main atmospheric parameters and abundances of the iron group elements (vanadium, chromium, iron, cobalt and nickel) are determined for 62 red giant "clump" stars revealed in the Galactic field by the Hipparcos orbiting observatory. The stars form a homogeneous sample with the mean value of temperature T=4750 +- 160K, of surface gravity log g = 2.41 +- 0.26 and the mean value of metallicity [Fe/H] = -0.04 +- 0.15 dex. A Gaussian fit to the [Fe/H] distribution produces the mean [Fe/H] = -0.01 dex and dispersion of [Fe/H] = 0.08 dex. The near-solar metallicity and small dispersion of [Fe/H] of clump stars of the Galaxy obtained in this work confirm the theoretical model of the Hipparcos clump by Girardi & Salaris (2001). This suggests that nearby clump stars are (in the mean) relatively young objects, reflecting mainly the near-solar metallicities developed in the local disk during the last few Gyrs of its history. We find iron group element to iron abundance ratios in clump giants to be close to solar.