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HE 1327-2326, An Unevolved Star With Fe/H < -5.0. II. New 3D-1D Corrected Abundances From A Very Large Telescope UVES Spectrum
(2008-09)
We present a new abundance analysis of HE 1327-2326, which is currently the most iron-poor star, based on observational data obtained with the VLT Ultraviolet and Visual Echelle Spectrograph (UVES). We correct the ...
The Milky Way Tomography With SDSS. II. Stellar Metallicity
(2008-09)
Using effective temperature and metallicity derived from SDSS spectra for similar to 60,000 F- and G-type main-sequence stars (0.2 < g - r < 0.6), we develop polynomial models for estimating these parameters from the SDSS ...
Rubidium And Lead Abundances In Giant Stars Of The Globular Clusters M4 And M5
(2008-02)
We present measurements of the neutron-capture elements Rb and Pb for bright giants in the globular clusters M4 and M5. The clusters are of similar metallicity ([Fe/ H] similar or equal to -1.2), but M4 is decidedly s-process ...