Lithium abundances of halo dwarfs (Hosford+, 2009)

Physics

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Stars: Dwarfs, Abundances

Scientific paper

Using high signal-to-noise (S/N~100) spectra of 16 metal-poor halo dwarfs, obtained with the UCLES spectrograph on the AAT, measurements of equivalent widths from a set of unblended FeI lines are made.
Table contains the wavelength, first column, of each line measured in the spectra of the program stars. Along with this there are the log(gf) values, the references for the log(gf) values and the excitation energy values for each spectral line, columns 2, 3 and 4 respectively. Following this we present the measured equivalent widths from the program stars, remaining columns.
(2 data files).

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