Derivation of stellar parameters and metallicity distributions using detailed spectroscopic analyses
A sample of 25 high resolution spectra of K and G type metal-poor giant located in thick disk of the Milky Way from the Space Interferometry Mission (SIM) Grid Planet Quest and 76 dwarf metal-rich stars selected from the Spectroscopic Survey of Stars in the Solar Neighborhood (S4N) are analyzed in order to derive fundamental stellar parameters (effective temperatures and surface gravities) and metallicity distributions by means of a Detailed Spectroscopic Analysis. ^
Physics, Astronomy and Astrophysics
Del Pardo, Cecilia, "Derivation of stellar parameters and metallicity distributions using detailed spectroscopic analyses" (2006). ETD Collection for University of Texas, El Paso. AAI1435345.