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CHEMICAL COMPOSITION OF INTERMEDIATE-MASS STAR MEMBERS OF THE M6 (NGC 6405) OPEN CLUSTER

  • Authors: T. Kılıçoğlu, R. Monier, J. Richer, L. Fossati, and B. Albayrak

2016 The Astronomical Journal 151 49.

  • Provider: AAS Journals

Caption: Figure 4.

Microturbulence determination by minimizing the standard deviation of [Fe/H].

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