Atmospheric parameters of nearby giant stars (Jones+, 2011)

Physics

Scientific paper

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Stars: Giant, Abundances: [Fe/H], Rotational Velocities, Spectroscopy

Scientific paper

We used high resolution and high S/N spectra to measure the equivalent widths of many FeI and FeII lines, which were used to derive the atmospheric parameters by imposing local thermodynamic and ionization equilibrium. The effective temperatures and metallicities were used, along with stellar evolutionary tracks to determine the physical properties and evolutionary status of each star.
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