Stellar abundance patterns. What is the possible level of completeness today
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G. Galazutdinov | F. Musaev | P. North | V. Gopka | A. Shavrina | A. Yushchenko | N. Polosukhina | C. Kim | Y. Pavlenko
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G. Galazutdinov | F. Musaev | P. North | V. Gopka | A. Shavrina | A. Yushchenko | N. Polosukhina | C. Kim | Y. Pavlenko