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Tracing Early Enrichment Pathways: Chemical and Chemodynamical Analysis of Two CEMP-no Stars

  • Authors: Meenakshi Purandardas

Meenakshi Purandardas 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 2.

The iron abundances of program stars as a function of excitation potential (left panels) and equivalent width (right panels). In all of the panels, the open circles indicate Fe I lines, and solid triangles represent Fe II lines.

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