Based on observations performed with European Southern Observatory (ESO) telescopes [programme IDs: 70.D-0081(A), 082.A-9007(A), 083.A-9011(B), 084.A-9011(B)].
Elemental abundances of low-mass stars in nearby young associations: AB Doradus, Carina Near and Ursa Major†
Article first published online: 26 NOV 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 427, Issue 4, pages 2905–2916, 21 December 2012
How to Cite
Biazzo, K., D'Orazi, V., Desidera, S., Covino, E., Alcalá, J. M. and Zusi, M. (2012), Elemental abundances of low-mass stars in nearby young associations: AB Doradus, Carina Near and Ursa Major. Monthly Notices of the Royal Astronomical Society, 427: 2905–2916. doi: 10.1111/j.1365-2966.2012.22132.x
- Issue published online: 26 NOV 2012
- Article first published online: 26 NOV 2012
- Manuscript Accepted: 13 SEP 2012
- Manuscript Received: 8 AUG 2012
- INAF Post-doctoral fellowship
- techniques: spectroscopic;
- stars: abundances;
- stars: individual: ι Horologii;
- open clusters and associations: individual: AB Doradus;
- open clusters and associations: individual: Carina Near;
- open clusters and associations: individual: Ursa Major
We present stellar parameters and abundances of 11 elements (Li, Na, Mg, Al, Si, Ca, Ti, Cr, Fe, Ni and Zn) of 13 F6–K2 main-sequence stars in the young groups AB Doradus, Carina Near and Ursa Major. The exoplanet-host star ι Horologii is also analysed.
The three young associations have lithium abundance consistent with their age. All other elements show solar abundances. The three groups are characterized by a small scatter in all abundances, with mean [Fe/H] values of 0.10 (σ = 0.03), 0.08 (σ = 0.05) and 0.01 (σ = 0.03) dex for AB Doradus, Carina Near and Ursa Major, respectively. The distribution of elemental abundances appears congruent with the chemical pattern of the Galactic thin disc in the solar vicinity, as found for other young groups. This means that the metallicity distribution of nearby young stars, targets of direct-imaging planet-search surveys, is different from that of old, field solar-type stars, i.e. the typical targets of radial velocity surveys.
The young planet-host star ι Horologii shows a lithium abundance lower than that found for the young association members. It is found to have a slightly super-solar iron abundance ([Fe/H] = 0.16 ± 0.09), while all [X/Fe] ratios are similar to the solar values. Its elemental abundances are close to those of the Hyades cluster derived from the literature, which seems to reinforce the idea of a possible common origin with the primordial cluster.