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1999AJ....117..981B - Astron. J., 117, 981-1009 (1999/February-0)
Estimation of stellar metal abundance. II. A recalibration of the Ca II K technique, and the autocorrelation function method.
BEERS T.C., ROSSI S., NORRIS J.E., RYAN S.G. and SHEFLER T.
Abstract (from CDS):
Metallicities based on a combination of the two techniques for dwarfs and giants in the color range 0.30≤(B-V)0≤1.2 exhibit an external 1 σ scatter of approximately 0.10-0.20 dex over the abundance range -4.0≤[Fe/H]≤0.5. Particular attention has been given to the determination of abundance estimates at the metal-rich end of the calibration, where our previous attempt suffered from a considerable zero-point offset. Radial velocities, accurate to approximately 10 km.s–1, are reported for all 551 calibration stars.
Abstract Copyright: ∼
Journal keyword(s): Galaxy: Abundances - Galaxy: Halo - Stars: Population II
VizieR on-line data: <Available at CDS (J/AJ/117/981): table4.dat table6.dat refs.dat>
CDS comments: Table 4 : NGC 6297 717 misprint of 6397 717. Stars in NGC 6752 are Cl* NGC 6752 CS, stars in M4 are Cl* NGC 6121 Lee, stars in M3 R-NNN are CL* NGC 5272 S R-R-NN (the first roman numeral, I for Serie I is omitted). Stars in M92 not identified.
Simbad objects: 547
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