S. F. A. Batista, V. Zh. Adibekyan, S. G. Sousa, N. C. Santos, E. Delgado Mena, A. A. Hakobyan
Abstract
The search for solar siblings has been particularly fruitful in the past few years. At present, there are four plausible candidates reported in the literature: HIP21158, HIP87382, HIP47399, and HIP92831. In this study we conduct a search for solar siblings among the HARPS high-resolution FGK dwarfs sample, which includes precise chemical abundances and kinematics for 1111 stars. Using a new approach based on chemical abundance trends with condensation temperature, kinematics, and ages we found one (additional) potential solar sibling candidate: HIP97507.
Keywords
stars: abundances - stars: kinematics and dynamics - solar neighborhood
Notes
Based on observations collected at the La Silla Paranal Observatory, ESO (Chile) with the HARPS spectrograph at the 3.6-m telescope (ESO runs ID 72.C-0488, 082.C-0212, and 085.C-0063).
Astronomy & Astrophysics
Volume 564, Number of pages A43_1
2014 April
