Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pkas...12..197l&link_type=abstract
Publications of the Korean Astronomical Society, vol.12, no.1, p.197-212
Astronomy and Astrophysics
Astronomy
Halo Stars, Photometric, Spectroscopic, And Kinematic Properties, Population Ii Stars
Scientific paper
The general photometric, spectroscopic, and kinematic properties of the late type halo stars are investigated from a sample of known true halo stars. Halo stars are distributed in a lower left region of infrared (J-H) vs (H-K) color-color diagram, which is reconfirmed to be useful for selection of halo stars. They move with average velocity components of 9km/sec, -14km/sec, and 5km/sec in U, V, and W directions respectively. They are distributed separately from disk stars in a diagram of metallicity index, CaH1/TiO5 vs (R-I).
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