The red giant metallicity function

Astronomy and Astrophysics – Astronomy

Scientific paper

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Metallicity, Red Giant Stars, Stellar Composition, Astronomical Photometry, Distribution Functions, Stellar Evolution

Scientific paper

For a sample of red giants comprising about 2000 stars the distributions of metallicity [Fe/H] are given. It is shown that they cannot be described by a gaussian one in the sense that the normal-law hypothesis turns out to be statistically insignificant, if the alternative is a hypothesis that the distribution is a sum of two normal curves. The center of the distributions of giants in both galactic poles is found to demonstrate a statistically significant gap similar to the one found earlier for the late main-sequence stars. The implications of the metallicity distribution properties for the problems of the chemical evolution of the galactic disk are discusssed.

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