Astronomy & Astrophysics manuscript no. zeta-reticuli c ESO 2018 July 9, 2018 ζ2 Ret, its debris disk, and its lonely stellar companion ζ1 Ret ? ?? Different Tc trends for different spectra , V. Adibekyan1, E. Delgado-Mena1, P. Figueira1, S. G. Sousa1, N. C. Santos1;2, J. P. Faria1;2, J. I. Gonzalez´ Hernandez´ 3;4, G. Israelian3;4, G. Harutyunyan5, L. Suarez-Andr´ es´ 3;4, and A. A. Hakobyan6 1 Instituto de Astrof´ısica e Cienciasˆ do Espac¸o, Universidade do Porto, CAUP, Rua das Estrelas, 4150-762 Porto, Portugal e-mail:
[email protected] 2 Departamento de F´ısica e Astronomia, Faculdade de Ciencias,ˆ Universidade do Porto, Rua do Campo Alegre, 4169-007 Porto, Portugal 3 Instituto de Astrof´ısica de Canarias, 38200 La Laguna, Tenerife, Spain 4 Departamento de Astrof´ısica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain 5 Leibniz Institute for Astrophysics Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany 6 Byurakan Astrophysical Observatory, 0213 Byurakan, Aragatsotn province, Armenia Received date / Accepted date ABSTRACT Context. Several studies have reported a correlation between the chemical abundances of stars and condensation temperature (known as Tc trend). Very recently, a strong Tc trend was reported for the ζ Reticuli binary system, which consists of two solar analogs. The observed trend in ζ2 Ret relative to its companion was explained by the presence of a debris disk around ζ2 Ret. Aims. Our goal is to re-evaluate the presence and variability of the Tc trend in the ζ Reticuli system and to understand the impact of the presence of the debris disk on a star.