Chemically tagging the Hyades Supercluster: A homogeneous sample of F6-K4 kinematically selected northern stars

TL;DR

This study uses chemical tagging to identify true members of the Hyades Supercluster, revealing that less than half of the candidates are genuine members and that the supercluster has a complex origin beyond the Hyades cluster.

Contribution

The paper presents a homogeneous chemical analysis of 61 stars to refine membership of the Hyades Supercluster using differential abundance analysis.

Findings

Only 28 out of 61 candidates are confirmed members.

The supercluster's origin is more complex than a single cluster.

Chemical abundances are consistent with Galactic trends.

Abstract

Stellar kinematic groups are kinematical coherent groups of stars that might have a common origin. These groups are dispersed throughout the Galaxy over time by the tidal effects of both Galactic rotation and disc heating, although their chemical content remains unchanged. The aim of chemical tagging is to establish that the abundances of every element in the analysis are homogeneus among the members. We study the case of the Hyades Supercluster to compile a reliable list of members (FGK stars) based on our chemical tagging analysis. For a total of 61 stars from the Hyades Supercluster, stellar atmospheric parameters (Teff, logg, xi, and [Fe/H]) are determined using our code called StePar, which is based on the sensitivity to the stellar atmospheric parameters of the iron EWs measured in the spectra. We derive the chemical abundances of 20 elements and find that their [X/Fe] ratios are consistent with Galactic abundance trends reported in previous studies. The chemical tagging method is applied with a carefully developed differential abundance analysis of each candidate member of the Hyades Supercluster, using a well-known member of the Hyades cluster as a reference (vB 153). We find that only 28 stars (26 dwarfs and 2 giants) are members, i.e. that 46% of our candidates are members based on the differential abundance analysis. This result confirms that the Hyades Supercluster cannot originate solely from the Hyades cluster.