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Metal-Deficient Giants in the Galactic Field - Catalogue and Some Physical Parameters Not Available
A kinematic and abundance survey at the galactic poles The DDO intermediate band system is used to obtain detailed informationabout abundance gradients and velocity dispersions in the galaxy, withan emphasis on the properties of halo stars in the range of from 1 to 5kpc. The DDO abundance index is calibrated agianst (Fe/H) for metal-poorstars, with a resulting gradient of about -0.2 per kpc. However, whenthe sample is divided into two subsamples with (Fe/H) less than -0.5 andequal to or greater than -0.5, the gradients are -0.14 and 0.00,respectively. DDO observations of about 1000 stars, mostly G5-K5 giants,show that the velocity dispersion increases both with decrease inmetallicity and increase in z distance. The abundances found for high-zstars are similar to the A-star results of Rodgers (1971) in that abouthalf the K giants above 1 kpc appear to have solar abundances.
Stellar population samples at the galactic poles. III - UBVRI observations of proper motion stars near the south pole and the luminosity laws for the halo and old disk populations Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1976ApJS...30..351E&db_key=AST

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Observation and Astrometry data

Constellation:	Γλύπτης
Right ascension:	01^h18^m56.44^s
Declination:	-29Â°57'32.9"
Apparent magnitude:	9.331
Proper motion RA:	100.3
Proper motion Dec:	68.6
B-T magnitude:	10.206
V-T magnitude:	9.404

Catalogs and designations:

Proper Names	(Edit)
HD 1989	HD 8000
TYCHO-2 2000	TYC 6427-931-1
USNO-A2.0	USNO-A2 0600-00506374
HIP	HIP 6151

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