| Issue |
A&A
Volume 564, April 2014
|
|
|---|---|---|
| Article Number | A43 | |
| Number of page(s) | 4 | |
| Section | Galactic structure, stellar clusters and populations | |
| DOI | https://doi.org/10.1051/0004-6361/201423645 | |
| Published online | 03 April 2014 | |
Research Note
Searching for solar siblings among the HARPS data⋆
1 Centro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal
e-mail: sergio.batista@astro.up.pt
2 Departamento de Física e Astronomia, Faculdade de Ciências da Universidade do Porto, 4169-007 Porto, Portugal
3 Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain
4 Byurakan Astrophysical Observatory, 0213 Byurakan, Aragatsotn province, Armenia
Received: 14 February 2014
Accepted: 6 March 2014
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.
Key words: stars: abundances / stars: kinematics and dynamics / solar neighborhood
© ESO, 2014
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