OI and FeII equivalent widths in metal-poor stars (Nissen+ 2002)

Physics

Scientific paper

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Stars: Dwarfs, Stars: Giant, Equivalent Widths

Scientific paper

The table gives equivalent widths (in mÅ) of OI and FeII lines for
35 metal-poor main sequence and subgiant stars as measured from high
resolution, high S/N spectra observed with the ESO VLT/UVES
spectrograph, during three observing runs: April 8-12, 2000, July 22-24,
2000, and April 10-12, 2001. (2 data files).

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