Abundances in the Local Region II: F, G, and K Dwarfs and Subgiants
Abstract
Parameters and abundances have been derived for 1002 stars of spectral types F, G, and K, and luminosity classes IV and V. After culling the sample for rotational velocity and effective temperature, 867 stars remain for discussion. Twenty-eight elements are considered in the analysis. The α, iron-peak, and Period 5 transition metal abundances for these stars show a modest enhancement over solar averaging about 0.05 dex. The lanthanides are more abundant, averaging about +0.2 dex over solar. The question is: Are these stars enhanced, or is the Sun somewhat metal-poor relative to these stars? The consistency of the abundances derived here supports an argument for the latter view. Lithium, carbon, and oxygen abundances have been derived. The stars show the usual lithium astration as a function of mass/temperature. There are more than 100 planet-hosts in the sample, and there is no discernible difference in their lithium content, relative to the remaining stars. The carbon and oxygen abundances show the well-known trend of decreasing [x/Fe] ratio with increasing [Fe/H].
- Publication:
-
The Astronomical Journal
- Pub Date:
- January 2017
- DOI:
- 10.3847/1538-3881/153/1/21
- arXiv:
- arXiv:1611.02897
- Bibcode:
- 2017AJ....153...21L
- Keywords:
-
- Galaxy: abundances;
- stars: abundances;
- stars: evolution;
- stars: fundamental parameters;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- 164 Pages 6 Tables (142 pages in the tables) 13 figures Accepted for publication - Astronomical Journal
