CCD photometry on the uvbyCa system has been obtained for 521 candidate metal-poor stars from the northern hemisphere HK survey of Beers and colleagues. Reddening corrections, classifications of stars by luminosity class, and the derivation of metal abundances based on Strömgren indices m 1 and hk are described and presented, along with preliminary spectroscopic estimates of abundance. A number of extremely metal-poor stars with [Fe/H] ≤ -2.50 are identified.
No takes yet. Share an insight, caveat, or question.
A 2000 study studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: