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Method for simultaneous determination of the metallicity and interstellar reddening of globular clusters using the <Emphasis Type="Italic">V</Emphasis> vs. (<Emphasis Type="Italic">B-R</Emphasis>) color-magnitude diagram
Authors:A N Gerashchenko
Institution:1.Pulkovo Astronomical Observatory,Russian Academy of Sciences,St. Petersburg,Russia
Abstract:We describe a method for simultaneous determination of the metallicity and interstellar reddening of globular clusters that uses parameters of the giant branch on the V vs. (B-R) color-magnitude diagram: the slope of the giant branch, its color at the level of the horizontal branch, and the apparent magnitude V of the horizontal branch. Applying this method to the globular cluster NGC 7006 gives the metallicity Fe/H] = −1.78 ± 0.11 and interstellar reddening E B-R = 0.25 ± 0.02.
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