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• W2001012873 abstract "We present a sample of 8321 candidate Field Horizontal-Branch (FHB) stars selected by automatic spectral classi- fication in the digital data base of the Hamburg/ESO objective-prism survey. The stars are distributed over 8225 square degrees of the southern sky, at |b| 30 deg. The average distance of the sample, assuming that they are all FHB stars, is 9.8 kpc, and distances of up to ∼30 kpc are reached. Moderate-resolution spectroscopic follow-up observations and UB V photometry of 125 test sample stars demonstrate that the contamination of the full candidate sample with main-sequence A-type stars is <16%, while it would be up to 50% in a flux-limited sample at high galactic latitudes. Hence more than ∼6800 of our FHB candidates are expected to be genuine FHB stars. The candidates are being used as distance probes for high-velocity clouds and for studies of the structure and kinematics of the Galactic halo." @default.
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• W2001012873 date "2005-02-01" @default.
• W2001012873 modified "2023-09-23" @default.
• W2001012873 title "The stellar content of the Hamburg/ESO survey. III. Field horizontal-branch stars in the Galaxy" @default.
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