The spectroscopic abundances and kinematics of a sample of faint B stars far from the galactic plane and appearing at the low spectroscopic dispersions to be Population I stars, were analyzed to determine their nature and origin. Out of 49 stars: 26 are identified as Population I stars that have been ejected from the galactic disk, 18 are evolved sub dwarfs, and 5 remain unclassified. There are no stars in the sample that appear to be Population I stars which formed in situ in the galactic halo.
This is a color reproduction of the mini-poster sheet I gave out at the meeting. Color copies of idividual figures are at the bottom of this page.
Here is where you can get the preprint on the eclipsing high galactic latitude binary IT Librae.
All 8.5 inch x 10 inch color landscape PDFs
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